질량이 큰 항성 목록: 두 판 사이의 차이

위키백과, 우리 모두의 백과사전.
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시각위키텍스트
태그: m 모바일 웹
편집 요약 없음
태그: nowiki 추가됨 구식 태그 m 모바일 웹
30번째 줄: 30번째 줄:


첫 번째 목록은 60&nbsp;{{태양질량}} 이상으로 추정되는 별으로 그 중 대부분이 수록되며 두 번째 목록에는 비교를 위해 60&nbsp;{{태양질량}} 미만의 주목할만한 별이 수록되어 있다. 데이터의 불확실성에 대한 정보를 제공하기 위해 각 별의 질량을 결정하는 데 사용되는 방법이 포함되어있으며 쌍성의 질량은 훨씬 더 정확하게 결정될 수 있다. 아래 나열된 질량은 별의 초기 질량이 아닌 현재 질량이다.{{미완성 목록|date=January 2016}}<!-- 삭제하지 마세요, 이 목록은 인류가 알려진 우주 전체를 관측하기 전에는 완성될 수 없습니다. -->
첫 번째 목록은 60&nbsp;{{태양질량}} 이상으로 추정되는 별으로 그 중 대부분이 수록되며 두 번째 목록에는 비교를 위해 60&nbsp;{{태양질량}} 미만의 주목할만한 별이 수록되어 있다. 데이터의 불확실성에 대한 정보를 제공하기 위해 각 별의 질량을 결정하는 데 사용되는 방법이 포함되어있으며 쌍성의 질량은 훨씬 더 정확하게 결정될 수 있다. 아래 나열된 질량은 별의 초기 질량이 아닌 현재 질량이다.{{미완성 목록|date=January 2016}}<!-- 삭제하지 마세요, 이 목록은 인류가 알려진 우주 전체를 관측하기 전에는 완성될 수 없습니다. -->

{| class="wikitable sortable"
{| class="wikitable sortable"
|+<big>'''60 {{태양질량|link=y}} 이상의 항성들'''<big>
|-
|-
! 항성 이름
! 항성 이름
! 질량<br>({{태양질량|link=on}}, [[태양]] = 1)
! [[질량]]
({{태양질량|link=y}}, [[태양]] = 1)
! 대략 태양계로부터의 거리([[광년]])
|-
! [[겉보기등급]]
|Westerhout 49-2
! [[표면온도|유효온도]] ([[켈빈|K]])
|250
! 분석 방식
|-
! 링크
|bgcolor="#9bb0ff"|[[BAT99-98]]<ref name="hainich">{{저널 인용
! 참고문헌
| doi = 10.1051/0004-6361/201322696
|- style="text-align:center;"
| title = The Wolf-Rayet stars in the Large Magellanic Cloud
| style="background: {{항성-색깔|WC}};text-align:left;" |[[BAT99-98]] (in [[타란툴라 성운]] of [[Large Magellanic Cloud|LMC]])
| journal = Astronomy & Astrophysics
| volume = 565
| pages = A27
| year = 2014
| last1 = Hainich | first1 = R.
| last2 = Rühling | first2 = U.
| last3 = Todt | first3 = H.
| last4 = Oskinova | first4 = L. M.
| last5 = Liermann | first5 = A.
| last6 = Gräfener | first6 = G.
| last7 = Foellmi | first7 = C.
| last8 = Schnurr | first8 = O.
| last9 = Hamann | first9 = W. -R.
| arxiv = 1401.5474
| bibcode = 2014A&A...565A..27H}}</ref>
|226
|226
|165,000
|-
|13.37
| bgcolor="#9bb0ff" |[[R136a1]]&nbsp;<ref name="crowther">{{저널 인용
|45,000
|last1=Crowther |first1=P. A.
|Spectroscopy
|last2=Schnurr |first2=O.
|{{SIMBAD link|BAT99+98|SIMBAD}}
|last3=Hirschi |first3=R.
|<ref name="hainich">{{cite journal |last1=Hainich |first1=R. |last2=Rühling |first2=U. |last3=Todt |first3=H.|last4=Oskinova|first4=L. M.|last5=Liermann|first5=A.|last6=Gräfener|first6=G.|last7=Foellmi|first7=C.|last8=Schnurr|first8=O.|last9=Hamann|first9=W.-R. |display-authors=6 |date=May 2014|title=The Wolf-Rayet stars in the Large Magellanic Cloud. A comprehensive analysis of the WN class |journal=Astronomy & Astrophysics |volume=565 |page=A27 |arxiv=1401.5474 |bibcode=2014A&A...565A..27H|doi=10.1051/0004-6361/201322696|issn=0004-6361|s2cid=55123954}}</ref><ref name="Doran2013">{{Cite journal |last1=Doran |first1=E.I. |last2=Crowther |first2=P.A.|last3=de Koter |first3=A. |last4=Evans |first4=C.J. |last5=McEvoy |first5=C. |last6=Walborn |first6=N.R. |last7=Bastian |first7=N. |last8=Bestenlehner |first8=J.M. |last9=Gräfener |first9=G. |last10=Herrero |first10=A. |last11=Köhler |first11=K. |first15=H. |first18=J.Th. |last19=Vink|last18=van Loon |first17=W.D. |last17=Taylor |first16=F.R.N. |last14=Puls |last16=Schneider |last15=Sana |first14=J. |first13=F. |last13=Najarro|first12=J. |last12=Maíz Apellániz |first19=J.S. |display-authors=6 |date=October 2013 |title=The VLT-FLAMES Tarantula Survey: XI. A census of the hot luminous stars and their feedback in 30 Doradus|journal=Astronomy & Astrophysics |volume=558 |page=A134 |arxiv=1308.3412 |bibcode=2013A&A...558A.134D|doi=10.1051/0004-6361/201321824 |issn=0004-6361 |s2cid=118510909}}</ref>
|last4=Yusof |first4=N.
|- style="text-align:center;"
|last5=Parker |first5=R. J.
| style="background: {{항성-색깔|WC}};text-align:left;" |[[R136a1]] (in [[타란툴라 성운]] of [[Large Magellanic Cloud|LMC]])
|last6=Goodwin |first6=S. P.
|last7=Kassim |first7=H. A.
|year=2010
|title=The R136 star cluster hosts several stars whose individual masses greatly exceed the accepted 150 M<sub>⊙</sub> stellar mass limit
|journal=Monthly Notices of the Royal Astronomical Society
|volume=408 |issue=2 |pages=731
|arxiv=1007.3284
|bibcode=2010MNRAS.408..731C
|doi=10.1111/j.1365-2966.2010.17167.x
}}</ref>
|196
|196
|163,000
|-
|12.23
|bgcolor="#9bb0ff"|[[BAT99-116]]<ref name="crowther"/>
|46,000
|190
|Evolution
|-
|{{SIMBAD link|RMC136a1|SIMBAD}}
|bgcolor="#9bb0ff"|[[R136a2]]&nbsp;<ref name="crowther"/>
|<ref name=":0">{{Cite journal |last1=Bestenlehner |first1=Joachim M. |last2=Crowther |first2=Paul A. |last3=Caballero-Nieves |first3=Saida M. |last4=Schneider |first4=Fabian R. N. |last5=Simón-Díaz |first5=Sergio |last6=Brands |first6=Sarah A. |last7=de Koter |first7=Alex |last8=Gräfener |first8=Götz |last9=Herrero |first9=Artemio |last10=Langer |first10=Norbert |last11=Lennon |first11=Daniel J. |date=2020-12-01 |title=The R136 star cluster dissected with Hubble Space Telescope/STIS - II. Physical properties of the most massive stars in R136 |url=https://ui.adsabs.harvard.edu/abs/2020MNRAS.499.1918B |journal=Monthly Notices of the Royal Astronomical Society |volume=499 |issue=2 |pages=1918–1936 |doi=10.1093/mnras/staa2801 |arxiv=2009.05136 |bibcode=2020MNRAS.499.1918B |issn=0035-8711}}</ref><ref name=":1">{{cite journal |last1=Kalari |first1=Venu M. |last2=Horch |first2=Elliott P. |last3=Salinas |first3=Ricardo |last4=Vink |first4=Jorick S. |last5=Andersen |first5=Morten |last6=Bestenlehner |first6=Joachim M. |last7=Rubio |first7=Monica |date=2022-07-26 |title=Resolving the Core of R136 in the Optical |journal=The Astrophysical Journal |volume=935 |issue=2 |page=162 |doi=10.3847/1538-4357/ac8424 |arxiv=2207.13078 |bibcode=2022ApJ...935..162K |s2cid=251067072 |doi-access=free }}</ref>
|179
|- style="text-align:center;"
|-
| style="background: {{항성-색깔|O}};text-align:left;" |[[멜닉 42]] (in [[타란툴라 성운]] of [[Large Magellanic Cloud|LMC]])
|bgcolor="#9bb0ff"|[[VFTS 682]]
|150
|189
|163,000
|-
|12.78
|bgcolor="#9bb0ff"|[[NGC 3603-B]]<ref name="crowther"/>
|47,300
|Spectroscopy
|{{SIMBAD link|Cl*+NGC+2070+MEL+42|SIMBAD}}
|<ref name="best">{{Cite journal |last1=Bestenlehner |first1=J.M. |last2=Gräfener |first2=G. |last3=Vink |first3=J.S. |last4=Najarro |first4=F. |last5=de Koter |first5=A. |last6=Sana |first6=H. |last7=Evans |first7=C.J. |last8=Crowther |first8=P.A. |last9=Hénault-Brunet |first9=V. |last10=Herrero |first10=A. |last11=Langer |first11=N. |last12=Schneider |first12=F.R.N. |last13=Simón-Díaz |first13=S. |first14=W.D. |last14=Taylor |first15=N.R. |last15=Walborn |display-authors=6 |date=October 2014 |title=The VLT-FLAMES Tarantula Survey: XVII. Physical and wind properties of massive stars at the top of the main sequence |journal=Astronomy & Astrophysics |volume=570 |page=A38 |arxiv=1407.1837 |bibcode=2014A&A...570A..38B |doi=10.1051/0004-6361/201423643 |issn=0004-6361 |s2cid=118606369}}</ref><ref name=Doran2013/>
|- style="text-align:center;"
| style="background: {{항성-색깔|WC}};text-align:left;" |[[VFTS 1022]] (in [[타란툴라 성운]] of [[Large Magellanic Cloud|LMC]])
|178
|164,000
|13.47
|42,200
|Spectroscopy
|{{SIMBAD link|VFTS+1022|SIMBAD}}
|<ref name=best/><ref name=Doran2013/>
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" |[[웨스터하우트 51]]-57 (in [[웨스터하우트 51]])
|160
|20,000
|16.66<br/>{{small|(J&nbsp;대역)}}
|42,700
|Evolution
|
|<ref name=Bik>{{Cite journal |last1=Bik |first1=A. |last2=Henning |first2=Th. |last3=Wu |first3=S.-W. |last4=Zhang |first4=M. |last5=Brandner |first5=W. |last6=Pasquali |first6=A. |last7=Stolte |first7=A. |date=April 2019 |title=Near-infrared spectroscopy of the massive stellar population of W51: evidence for multi-seeded star formation |journal=Astronomy & Astrophysics |volume=624 |page=A63 |arxiv=1902.05460 |bibcode=2019A&A...624A..63B |doi=10.1051/0004-6361/201935061 |issn=0004-6361 |s2cid=118711844 }}</ref>
|- style="text-align:center;"
| style="background: {{항성-색깔|WC}};text-align:left;" |[[R136a3]] (in [[타란툴라 성운]] of [[Large Magellanic Cloud|LMC]])
|155
|163,000
|12.97
|50,000
|Evolution
|{{SIMBAD link|RMC136a3|SIMBAD}}
|<ref name=":0" /><ref name=":1"/>
|- style="text-align:center;"
| style="background: {{항성-색깔|WC}};text-align:left;" |[[VFTS 682]] (in [[타란툴라 성운]] of [[Large Magellanic Cloud|LMC]])
|153
|164,000
|16.08
|52,200
|Spectroscopy
|{{SIMBAD link|VFTS+682|SIMBAD}}
|<ref name="bagnulo2020">{{Cite journal|last1=Bagnulo |first1=S. |last2=Wade |first2=G.A. |last3=Nazé |first3=Y. |last4=Grunhut |first4=J.H. |last5=Shultz |first5=M.E. |last6=Asher |first6=D.J. |last7=Crowther |first7=P.A. |last8=Evans |first8=C.J. |last9=David-Uraz |first9=A. |last10=Howarth |first10=I.D. |last11=Morrell |first11=N. |last12=Munoz |first12=M.S. |last13=Neiner |first13=C. |last14=Puls |first14=J. |last15=Szymański |first15=M.K. |last16=Vink |first16=J.S. |display-authors=6 |date=March 2020|title=A search for strong magnetic fields in massive and very massive stars in the Magellanic Clouds|journal=Astronomy & Astrophysics |volume=635 |page=A163 |arxiv=2002.12061 |bibcode=2020A&A...635A.163B |doi=10.1051/0004-6361/201937098 |issn=0004-6361|s2cid=211532767}}</ref><ref name="Doran2013" />
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" |[[HD 15558]] A (in [[IC 1805]] of [[Heart Nebula]])
|152
|24,400
|7.87<br/>{{small|(연성계 전체)}}
|39,500
|Binary
|{{SIMBAD link|HD+15558|SIMBAD}}
|<ref name="debecker">{{Cite journal|last1=De Becker |first1=M. |last2=Rauw |first2=G. |last3=Manfroid |first3=J. |last4=Eenens |first4=P. |date=September 2006 |title=Early-type stars in the young open cluster IC&nbsp;1805: II. The probably single stars HD&nbsp;15570 and HD&nbsp;15629, and the massive binary/triple system HD&nbsp;15558 |journal=Astronomy & Astrophysics |volume=456 |issue=3 |pages=1121–1130 |arxiv=astro-ph/0606379 |bibcode=2006A&A...456.1121D |doi=10.1051/0004-6361:20065300|issn=0004-6361|s2cid=16519684}}</ref><ref name=ducati>{{cite report |last1=Ducati |first1=J.R. |year=2002 |title=VizieR Online Data Catalog: Catalogue of Stellar Photometry in Johnson's 11-color system |publisher=CDS/ADC |series=Collection of Electronic Catalogues |volume=2237 |bibcode=2002yCat.2237....0D |s2cid=118191108}}</ref>
|- style="text-align:center;"
| style="background: {{항성-색깔|WC}};text-align:left;" |[[R136a2]] (in [[타란툴라 성운]] of [[Large Magellanic Cloud|LMC]])
|151
|163,000
|12.34
|50,000
|Evolution
|{{SIMBAD link|RMC136a2|SIMBAD}}
|<ref name=":0"/><ref name=":1"/>
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" |[[웨스터하우트 51]]-3 (in [[웨스터하우트 51]])
|148
|20,000
|17.79<br/>{{small|(J&nbsp;대역)}}
|39,800
|Evolution
|{{SIMBAD link|2MASS+J19234283%2B1430277|SIMBAD}}
|<ref name=Bik/>
|- style="text-align:center;"
| style="background: {{항성-색깔|WC}};text-align:left;" |[[멜닉 34]] A (in [[타란툴라 성운]] of [[Large Magellanic Cloud|LMC]])
|147
|163,000
|13.09<br/>{{small|(연성계 전체)}}
|53,000
|Binary
|{{SIMBAD link|Cl*+NGC+2070+MEL+34|SIMBAD}}
|<ref name="tehrani">{{Cite journal |last1=Tehrani |first1=Katie A. |last2=Crowther |first2=Paul A. |last3=Bestenlehner |first3=Joachim M. |last4=Littlefair|first4=Stuart P. |last5=Pollock |first5=A.M.T. |last6=Parker |first6=Richard J. |last7=Schnurr |first7=Olivier |date=1 April 2019 |title=Weighing Melnick&nbsp;34: the most massive binary system known |journal=Monthly Notices of the Royal Astronomical Society |lang=en |volume=484 |issue=2 |pages=2692–2710 |arxiv=1901.04769 |bibcode=2019MNRAS.484.2692T|doi=10.1093/mnras/stz147|issn=0035-8711|s2cid=119069481}}</ref><ref name="Doran2013" />
|- style="text-align:center;"
| style="background: {{항성-색깔|WC}};text-align:left;" |[[VFTS 482]] (in [[타란툴라 성운]] of [[Large Magellanic Cloud|LMC]])
|145
|164,000
|12.95
|42,200
|Spectroscopy
|{{SIMBAD link|VFTS+482|SIMBAD}}
|<ref name="best"/><ref name="Doran2013" />
|- style="text-align:center;"
| style="background: {{항성-색깔|WC}};text-align:left;" |[[R136c]] (in [[타란툴라 성운]] of [[Large Magellanic Cloud|LMC]])
|142
|163,000
|13.43
|51,000
|Evolution
|{{SIMBAD link|RMC136c|SIMBAD}}
|<ref name="schneider2018">{{Cite journal |last1=Schneider |first1=F.R.N. |last2=Sana |first2=H. |last3=Evans |first3=C.J. |last4=Bestenlehner |first4=J.M. |last5=Castro |first5=N. |last6=Fossati |first6=L. |last7=Gräfener |first7=G. |last8=Langer |first8=N. |last9=Ramírez-Agudelo |first9=O.H. |last10=Sabín-Sanjulián |first10=C. |last11=Simón-Díaz |first11=S. |last12=Tramper |first12=F. |last13=Crowther |first13=P.A. |last14=de Koter |first14=A. |last15=de Mink |first15=S.E. |last16=Dufton |first16=P.L. |last17=Garcia |first17=M. |last18=Gieles |first18=M. |last19=Hénault-Brunet |first19=V. |last20=Herrero |first20=A. |last21=Izzard |first21=R.G. |last22=Kalari |first22= V. |last23=Lennon |first23= D.J. |last24=Maíz Apellániz |first24=J. |last25=Markova |first25=N. |last26=Najarro |first26=F. |last27=Podsiadlowski |first27=Ph. |last28=Puls |first28=J. |last29=Taylor |first29= W.D. |last30=van Loon |first30= J.Th. |last31=Vink |first31=J.S. |last32=Norman |first32=C. |display-authors=6 |date=5 January 2018 |title=An excess of massive stars in the local 30 Doradus starburst |journal=Science |language=en |volume=359 |issue=6371 |pages=69–71 |arxiv=1801.03107|bibcode=2018Sci...359...69S |doi=10.1126/science.aan0106 |pmid=29302009 |issn=0036-8075 |s2cid=206658504}}</ref><ref name="Doran2013" />
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" |[[VFTS 1021]] (in [[타란툴라 성운]] of [[Large Magellanic Cloud|LMC]])
|141
|164,000
|13.35
|39,800
|Spectroscopy
|{{SIMBAD link|VFTS+1021|SIMBAD}}
|<ref name="best" /><ref name="Doran2013" />
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" |[[LH 10]]-3209 A (in [[NGC 1763]] of [[Large Magellanic Cloud|LMC]])
|140
|160,000
|11.859<br/>{{small|(연성계 전체)}}
|42,500
|Spectroscopy
|{{SIMBAD link|PGMW+3209|SIMBAD}}
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|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" |[[VFTS 506]] (in [[타란툴라 성운]] of [[Large Magellanic Cloud|LMC]])
|138
|164,000
|13.31
|47,300
|Spectroscopy
|{{SIMBAD link|VFTS+506|SIMBAD}}
|<ref name="bagnulo2020"/><ref name="Doran2013" />
|- style="text-align:center;"
| style="background: {{항성-색깔|WC}};text-align:left;" |[[멜닉 34]] B (in [[타란툴라 성운]] of [[Large Magellanic Cloud|LMC]])
|136
|163,000
|13.09<br/>{{small|(연성계 전체)}}
|53,000
|Binary
|{{SIMBAD link|Cl*+NGC+2070+MEL+34|SIMBAD}}
|<ref name="tehrani" /><ref name="Doran2013" />
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" |[[웨스터하우트 51]]<nowiki/>d (in [[웨스터하우트 51]])
|135
|20,000
|15.11<br/>{{small|(J&nbsp;대역)}}
|42,700
|Evolution
|
|<ref name=Bik/>
|- style="text-align:center;"
| style="background: {{항성-색깔|WC}};text-align:left;" |[[VFTS 545]] (in [[Tarantula Nebula]] of [[Large Magellanic Cloud|LMC]])
|133
|164,000
|13.32
|47,300
|Spectroscopy
|{{SIMBAD link|VFTS+545|SIMBAD}}
|<ref name="best" /><ref name="Doran2013"/>
|- style="text-align:center;"
| style="background: {{항성-색깔|WC}};text-align:left;" |[[NGC 3603-B|HD 97950 B]] (WR 43b in [[HD 97950]] of [[NGC 3603]])
|132
|132
|24,800
|-
|11.33
|bgcolor="#9bb0ff"|[[R136c]]
|42,000
|≥130
|Spectroscopy
|-
|{{SIMBAD link|HD+97950B|SIMBAD}}
|bgcolor="#9bb0ff"|[[R136a3]]&nbsp;<ref name="hainich"/>
|<ref name="crowther">{{cite journal |last1=Crowther |first1=Paul A. |last2=Schnurr |first2=Olivier |last3=Hirschi|first3=Raphael |last4=Yusof |first4=Norhasliza|last5=Parker |first5=Richard J. |last6=Goodwin |first6=Simon P. |last7=Kassim |first7=Hasan Abu |date=21 October 2010|title=The R136 star cluster hosts several stars whose individual masses greatly exceed the accepted 150 M⊙ stellar mass limit|journal=Monthly Notices of the Royal Astronomical Society|language=en|volume=408|issue=2|pages=731–751|arxiv=1007.3284|bibcode=2010MNRAS.408..731C|doi=10.1111/j.1365-2966.2010.17167.x|issn=0035-8711|s2cid=53001712}}</ref><ref name="melena2008">{{Cite journal |last1=Melena |first1=Nicholas W. |last2=Massey|first2=Philip|last3=Morrell|first3=Nidia I. |last4=Zangari |first4=Amanda M. |date=1 March 2008 |title=The massive star content of NGC 3603 |journal=[[The Astronomical Journal]] |volume=135 |issue=3 |pages=878–891 |arxiv=0712.2621 |bibcode=2008AJ....135..878M |doi=10.1088/0004-6256/135/3/878 |issn=0004-6256|s2cid=16765414}}</ref>
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" |[[HD 269810]] (in [[NGC 2029]] of [[Large Magellanic Cloud|LMC]])
|130
|130
| 163,000
|-
|12.22
|bgcolor="#aabfff"|[[HD 269810]]
|52,500
|130
|Spectroscopy
|-
|{{SIMBAD link|HD+269810|SIMBAD}}
|bgcolor="#9bb0ff"|[[WR 42e]]<ref name=ejected>[http://arxiv.org/abs/1211.5926v1 Two massive stars possibly ejected from NGC 3603 via a three-body encounter], V. V. Gvaramadze, A. Y. Kniazev, A.-N. Chene, O. Schnurr, Submitted on 26 Nov 2012, 2015-04-14 확인.</ref>
|<ref name="evans">{{Cite journal |last1=Evans|first1=C.J. |last2=Walborn |first2=N.R. |last3=Crowther |first3=P.A. |last4=Hénault-Brunet |first4=V. |last5=Massa |first5=D. |last6=Taylor |first6=W.D.|last7=Howarth|first7=I.D. |last8=Sana |first8=H. |last9=Lennon |first9=D.J. |last10=van Loon |first10=J Th. |display-authors=6 |date=1 June 2010 |title=A massive runaway star from 30 Doradus |journal=The Astrophysical Journal|volume=715|issue=2|pages=L74–L79|arxiv=1004.5402|bibcode=2010ApJ...715L..74E|doi=10.1088/2041-8205/715/2/L74|issn=2041-8205|s2cid=118498849}}</ref><ref name="zacharias">{{Cite journal |last1=Zacharias |first1=N. |last2=Finch |first2=C.T. |last3=Girard |first3=T.M. |last4=Henden |first4=A. |last5=Bartlett |first5=J.L.|author5-link=Jennifer Bartlett (astronomer) |last6=Monet|first6=D.G.|last7=Zacharias |first7=M.I. |date=July 2012 |title=VizieR On-Line Data Catalog: UCAC4 Catalogue|journal=VizieR On-Line Data Catalog: I/322A. Originally Published in: 2012yCat.1322....0Z; 2013AJ....145...44Z|volume=1322|bibcode=2012yCat.1322....0Z|s2cid=211646126}}</ref>
|125-135<ref group=a>이 값은 NGC 3603 내 천체 3개가 상호작용하던 중 이 항성이 계를 이탈했다는 가정하에 나온 것이다. 이 항성은 천체 3개 중 근접쌍성 두 개가 하나로 합쳐진 것이다. 이 값은 이론상 비슷한 질량의 항성이 진화과정을 겪었다고 가정했을 때의 잔여질량과 일치한다.</ref>
|- style="text-align:center;"
|-
| style="background: {{항성-색깔|O}};text-align:left;" |[[R136|R136a7]] (in [[Tarantula Nebula]] of [[Large Magellanic Cloud|LMC]])
|bgcolor="#9bb0ff"|[[아치스 성단|아치스]]-F9
|127
|111–131
|163,000
|-
|13.97
|bgcolor="#9bb0ff"|[[NGC 3603-A1]]a
|54,000
|Evolution
|{{SIMBAD link|RMC136a7|SIMBAD}}
|<ref name="Brands2022">{{Cite journal |last1=Brands |first1=S. |last2=de Koter |first2=A. |last3=Bestenlehner |first3=J. |last4=Crowther |first4=P. |last5=Sundqvist |first5=J. |last6=Puls |first6=J. |last7=Caballero-Nieves |first7=S. |last8=Abdul-Masih |first8=M. |last9=Driessen |first9=F. |last10=Garcia |first10=M. |last11=Geen |first11=S. |display-authors=6 |date=7 April 2022 |title=The R136 star cluster dissected with Hubble Space Telescope/STIS. III. The most massive stars and their clumped winds |url=https://www.aanda.org/10.1051/0004-6361/202142742 |journal=Astronomy & Astrophysics |arxiv=2202.11080 |bibcode=2022A&A...663A..36B |doi=10.1051/0004-6361/202142742 |issn=0004-6361 |last12=Gräfener |first12=G. |last13=Hawcroft |first13=C. |last14=Kaper |first14=L. |last15=Keszthelyi |first15=Z. |last16=Langer |first16=N. |last17=Sana |first17=H. |last18=Schneider |first18=Fabian R. N. |last19=Shenar |first19=T. |last20=Vink |first20=Jorick S. |volume=663 |page=A36 |s2cid=247025548}}</ref><ref name="Doran2013" />
|- style="text-align:center;"
| style="background: {{항성-색깔|WC}};text-align:left;" |[[WR 42e]] (in [[HD 97950]] of [[NGC 3603]])
|123
|25,000
|14.53
|43,000
|Ejection
|{{SIMBAD link|WR+42e|SIMBAD}}
|<ref name=soar>{{Cite journal |last1=Roman-Lopes |first1=A. |last2=Franco|first2=G.A.P. |last3=Sanmartim |first3=D. |date=26 May 2016 |title=SOAR Optical and Near-infrared Spectroscopic Survey of Newly Discovered Massive Stars in the Periphery of Galactic Massive Star Clusters I-NGC 3603|journal=The Astrophysical Journal |volume=823 |issue=2 |page=96 |arxiv=1604.01096 |bibcode=2016ApJ...823...96R |doi=10.3847/0004-637X/823/2/96 |issn=1538-4357 |s2cid=119204619 |doi-access=free }}</ref>{{efn|This unusual measurement was made by assuming the star was ejected from a three-body encounter in NGC 3603. This assumption also means that the current star is the result of a merger between two original close binary components. The mass is consistent with evolutionary mass for a star with the observed parameters.}}
|- style="text-align:center;"
| style="background: {{항성-색깔|WC}};text-align:left;" |[[NGC 3603-A1|HD 97950 A1a]] (WR 43a A in [[HD 97950]] of [[NGC 3603]])
|120
|24,800
|11.18<br/>{{small|(연성계 전체)}}
|42,000
|Binary
|{{SIMBAD link|Cl*+NGC+3603+BLW+A1|SIMBAD}}
|<ref name="crowther" /><ref name="melena2008" />
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" |[[LSS 4067]] (in [[HM 1]])
|120
|11,000
|11.44
|40,000
|Evolution
|{{SIMBAD link|LSS+4067|SIMBAD}}
|<ref name=Massey2001>{{cite journal |last1=Massey |first1=Philip |last2=DeGioia-Eastwood |first2=Kathleen|author2-link=Kathy Eastwood |last3=Waterhouse |first3=Elizabeth |date=February 2001 |title=The progenitor masses of Wolf-Rayet stars and luminous blue variables determined from cluster turnoffs. II. Results from 12&nbsp;galactic clusters and OB associations |journal=The Astronomical Journal |volume=121 |issue=2 |pages=1050–1070 |arxiv=astro-ph/0010654 |bibcode=2001AJ....121.1050M |doi=10.1086/318769 |issn=0004-6256 |s2cid=53345173}}</ref><ref name="Vazquez">{{cite journal |last1=Vázquez |first1=R.A. |last2=Baume |first2=G. |date=June 2001 |title=The open cluster Havlen-Moffat no.&nbsp;1 revisited |journal=Astronomy & Astrophysics |volume=371 |issue=3 |pages=908–920 |bibcode=2001A&A...371..908V |doi=10.1051/0004-6361:20010410 |issn=0004-6361 |s2cid=121918776|doi-access=free }}</ref>
|- style="text-align:center;"
| style="background: {{항성-색깔|WC}};text-align:left;" |[[피스미스 24|WR 93]] (in [[피스미스 24]] of [[NGC 6357]])
|120
|120
|5,900
|-
|10.68
|bgcolor="#aabfff"|[[용골자리 에타]] A
|71,000
|125±25
|Evolution
|-
|{{SIMBAD link|WR+93|SIMBAD}}
|bgcolor="#9bb0ff"|[[R136b]]
|<ref name=Massey2001/><ref name=ducati/>
|118
|- style="text-align:center;"
|-
| style="background: {{항성-색깔|O}};text-align:left;" |[[Sk -69° 212]] (in [[NGC 2044]] of [[Large Magellanic Cloud|LMC]])
|bgcolor="#aabfff"|[[HD 93250]]
|118
|119
|160,000
|-
|12.416
|bgcolor="#aabfff"|[[R145]]<ref name=schnurr>{{저널 인용
|45,400
| last1 = Schnurr | first1 = O.
|Evolution
| last2 = Moffat | first2 = A. F. J.
|{{SIMBAD link|Sk+-69+212|SIMBAD}}
| last3 = Villar-Sbaffi | first3 = A.
|<ref name=Massey2000>{{cite journal |last1=Massey|first1=Philip |last2=Waterhouse |first2=Elizabeth |last3=DeGioia-Eastwood |first3=Kathleen |author3-link=Kathy Eastwood|date=May 2000 |title=The progenitor masses of Wolf-Rayet stars and luminous blue variables determined from cluster turnoffs. I. Results from 19&nbsp;OB&nbsp;associations in the Magellanic Clouds |journal=The Astronomical Journal |volume=119 |issue=5 |pages=2214–2241 |arxiv=astro-ph/0002233 |bibcode=2000AJ....119.2214M |doi=10.1086/301345 |issn=0004-6256 |s2cid=16891188}}</ref><ref name=Bonanos/>
| last4 = St-Louis | first4 = N.
|- style="text-align:center;"
| last5 = Morrell | first5 = N. I.
| style="background: {{항성-색깔|O}};text-align:left;" |[[Sk -69° 249]] A (in [[NGC 2074]] of [[Large Magellanic Cloud|LMC]])
| title = A first orbital solution for the very massive 30 Dor main-sequence WN6h+O binary R145
|119
| doi = 10.1111/j.1365-2966.2009.14437.x
|160,000
| journal = Monthly Notices of the Royal Astronomical Society
|12.02<br/>{{small|(연성계 전체)}}
| volume = 395
|38,900
| issue = 2
|Evolution
| pages = 823
|{{SIMBAD link|Sk+-69+249|SIMBAD}}
| year = 2009
|<ref name=Massey2000/><ref name=Tycho2>{{Cite journal |last1=Fabricius |first1=C. |last2=Høg |first2=E. |last3=Makarov |first3=V.V. |last4=Mason |first4=B.D. |last5=Wycoff |first5=G.L. |last6=Urban |first6=S.E. |date=March 2002 |title=The Tycho double star catalogue |journal=Astronomy & Astrophysics |volume=384|issue=1|pages=180–189 |bibcode=2002A&A...384..180F |doi=10.1051/0004-6361:20011822 |issn=0004-6361 |s2cid=56060737|doi-access=free }}</ref>
| pmid =
|- style="text-align:center;"
| pmc =
| style="background: {{항성-색깔|O}};text-align:left;" |[[ST5-31]] (in [[NGC 2074]] of [[Large Magellanic Cloud|LMC]])
|arxiv = 0901.0698 |bibcode = 2009MNRAS.395..823S }}</ref>
|119
|>116 + >48<ref group=a>현재 이 항성계의 궤도요소가 정확히 밝혀지지 않았기 때문에 질량은 최솟값이다.</ref>
|160,000
|-
|12.273
|bgcolor="#aabfff"|[[백조자리 OB2]]-7
|50,700
|Evolution
|{{SIMBAD link|ST92+5-31|SIMBAD}}
|<ref name=Massey2000/><ref name=Zaritsky>{{Cite journal |last1=Zaritsky |first1=Dennis |last2=Harris |first2=Jason |last3=Thompson |first3=Ian B. |last4=Grebel |first4=Eva K. |date=October 2004 |title=The Magellanic Clouds Photometric Survey: The Large Magellanic Cloud Stellar Catalog and Extinction Map |journal=The Astronomical Journal |language=en |volume=128 |issue=4 |pages=1606–1614 |arxiv=astro-ph/0407006 |bibcode=2004AJ....128.1606Z |doi=10.1086/423910 |issn=0004-6256 |s2cid=119532934}}</ref>
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" |[[R136|R136a5]] (in [[Tarantula Nebula]] of [[Large Magellanic Cloud|LMC]])
|116
|157,000
|13.71
|48,000
|Evolution
|{{SIMBAD link|RMC136a5|SIMBAD}}
|<ref name="Brands2022" /><ref name=Doran2013/>
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" |[[MSP 183]] (in [[웨스터룬드 2]])
|115
|20,000
|13.878
|46,300
|Spectroscopy
|{{SIMBAD link|Cl*+Westerlund+2+MSP+183|SIMBAD}}
|<ref>{{Cite journal |last1=Drew |first1=J.E. |last2=Herrero |first2=A. |last3=Mohr-Smith |first3=M. |last4=Monguió |first4=M. |last5=Wright |first5=N.J. |last6=Kupfer |first6=T. |last7=Napiwotzki |first7=R. |date=21 October 2018 |title=Massive stars in the hinterland of the young cluster, Westerlund&nbsp;2 |journal=Monthly Notices of the Royal Astronomical Society |lang=en |volume=480 |issue=2 |pages=2109–2124 |arxiv=1807.06486 |bibcode=2018MNRAS.480.2109D |doi=10.1093/mnras/sty1905 |issn=0035-8711 |s2cid=53126230}}</ref><ref>{{Cite journal |last1=Vargas Álvarez |first1=Carlos A. |last2=Kobulnicky |first2=Henry A. |last3=Bradley |first3=David R. |last4=Kannappan |first4=Sheila J. |last5=Norris |first5=Mark A. |last6=Cool |first6=Richard J. |last7=Miller |first7=Brendan P. |date=25 March 2013 |title=The distance to the massive galactic cluster Westerlund&nbsp;2 from a spectroscopic and HST photometric study |journal=The Astronomical Journal |volume=145 |issue=5 |page=125 |arxiv=1302.0863 |bibcode=2013AJ....145..125V |doi=10.1088/0004-6256/145/5/125 |issn=0004-6256|s2cid=67769122}}</ref>
|- style="text-align:center;"
| style="background: {{항성-색깔|WC}};text-align:left;" |[[WR 24]] (in [[콜린더 228]] of [[용골자리 성운]])
|114
|114
|14,000
|-
| style="background:lightblue;color:darkblue;" |'''6.48'''
|bgcolor="#9bb0ff"|[[NGC 3603]]-C<ref name="crowther"/>
|50,100
|Evolution
|{{SIMBAD link|WR+24|SIMBAD}}
|<ref name="hamann2019">{{cite journal |last1=Hamann |first1=W.-R. |last2=Gräfener |first2=G. |last3=Liermann |first3=A. |last4=Hainich |first4=R. |last5=Sander |first5=A.a.C. |last6=Shenar |first6=T. |last7=Ramachandran |first7=V. |last8=Todt |first8=H. |last9=Oskinova |first9=L.M. |display-authors=6 |date=1 May 2019 |title=The galactic WN&nbsp;stars revisited - impact of Gaia distances on fundamental stellar parameters |journal=Astronomy & Astrophysics |language=en |volume=625 |page=A57 |arxiv=1904.04687 |bibcode=2019A&A...625A..57H |doi=10.1051/0004-6361/201834850|issn=0004-6361|s2cid=104292503}}</ref><ref name="gcvs">{{cite journal |last1=Samus |first1=N.N. |last2=Kazarovets |first2=E.V. |last3=Durlevich |first3=O.V. |last4=Kireeva |first4=N.N. |last5=Pastukhova |first5=E.N. |date=January 2009 |title=VizieR Online Data Catalog: General Catalogue of Variable Stars (Samus+ 2007-2013) |journal=VizieR On-Line Data Catalog: B/GCVS. Originally Published in: 2017ARep...61...80S; 2017AZh....94...87S |volume=1 |bibcode=2009yCat....102025S |s2cid=208116145}}</ref>
|- style="text-align:center;"
| style="background: {{항성-색깔|WC}};text-align:left;" | [[NGC 3603-C|HD 97950 C]]1 (WR 43c A in [[HD 97950]] of [[NGC 3603]])
|113
|113
|24,800
|-
|11.89<br/>{{small|(연성계 전체)}}
|bgcolor="#9bb0ff"|[[멜닉 42]]
|44,000
|113
|Spectroscopy
|-
|{{SIMBAD link|HD+97950C|SIMBAD}}
|bgcolor="#cad8ff"|[[백조자리 OB2-12]]
|<ref name=crowther/><ref name=melena2008/><ref group="lower-alpha" name="Binary">This is a binary system but the secondary is much less massive than the primary.</ref>
|- style="text-align:center;"
| style="background: {{항성-색깔|WC}};text-align:left;" |[[아치스 성단|아치스]]-F9 (WR 102ae in [[아치스 성단]])
|111.3
|25,000
|16.1<br/>{{small|(J&nbsp;대역)}}
|36,600
|Spectroscopy
|{{SIMBAD link|FNG2002+9|SIMBAD}}
|<ref name="grafener">{{Cite journal |last1=Gräfener |first1=G. |last2=Vink |first2=J.S. |last3=de&nbsp;Koter |first3=A. |last4=Langer |first4=N. |date=November 2011 |title=The Eddington factor as the key to understand the winds of the most massive stars: Evidence for a Γ-dependence of Wolf-Rayet type mass loss |journal=Astronomy & Astrophysics |volume=535 |page=A56 |arxiv=1106.5361 |bibcode=2011A&A...535A..56G |doi=10.1051/0004-6361/201116701 |issn=0004-6361 |s2cid=59396651}}</ref><ref name=Figer>{{Cite journal|last1=Figer|first1=Donald F.|last2=Najarro|first2=Francisco|last3=Gilmore|first3=Diane|last4=Morris|first4=Mark|last5=Kim|first5=Sungsoo S.|last6=Serabyn|first6=Eugene|last7=McLean|first7=Ian S.|last8=Gilbert|first8=Andrea M.|last9=Graham|first9=James R.|last10=Larkin|first10=James E.|last11=Levenson|first11=N.A. |display-authors=6 |date=10 December 2002|title=Massive Stars in the Arches Cluster|journal=The Astrophysical Journal|language=en|volume=581|issue=1|pages=258–275|arxiv=astro-ph/0208145|bibcode=2002ApJ...581..258F|doi=10.1086/344154|issn=0004-637X|s2cid=119002004|last12=Harry I.|first12=Teplitz}}</ref>
|- style="text-align:center;"
| style="background: {{항성-색깔|B}};text-align:left;" |[[백조자리 OB2-12|백조자리 OB2 #12]] A (in [[백조자리 OB2]])
|110
|110
|5,200
|-
|11.702<br/>{{small|(연성계 전체)}}
|bgcolor="#9bb0ff"|[[WR 25]]
|13,700
|Spectroscopy
|{{SIMBAD link|Cyg+OB2+12|SIMBAD}}
|<ref name="clark">{{Cite journal|last1=Clark|first1=J. S.|last2=Najarro|first2=F.|last3=Negueruela|first3=I.|last4=Ritchie|first4=B. W.|last5=Urbaneja|first5=M. A.|last6=Howarth|first6=I. D.|date=May 2012|title=On the nature of the galactic early-B hypergiants|journal=Astronomy & Astrophysics|volume=541|page=A145|arxiv=1202.3991|bibcode=2012A&A...541A.145C|doi=10.1051/0004-6361/201117472|issn=0004-6361|s2cid=11978733}}</ref><ref name=Laur>{{Cite journal|last1=Laur|first1=Jaan|last2=Kolka|first2=Indrek|last3=Eenmäe|first3=Tõnis|last4=Tuvikene|first4=Taavi|last5=Leedjärv|first5=Laurits|date=February 2017|title=Variability survey of brightest stars in selected OB associations|journal=Astronomy & Astrophysics|volume=598|page=A108|arxiv=1611.02452|bibcode=2017A&A...598A.108L|doi=10.1051/0004-6361/201629395|issn=0004-6361|s2cid=119076598}}</ref><ref group=lower-alpha name=Binary/>
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" |[[HD 93129]] Aa (in [[트럼플러 14]] of [[용골자리 성운]])
|110
|110
|7,500
|-
|6.9<br/>{{small|(연성계 전체)}}
|bgcolor="#9bb0ff"|[[아치스 성단|아치스]]-F1
|42,500
|101–119
|Trinary
|-
|{{SIMBAD link|HD+93129A|SIMBAD}}
|bgcolor="#9bb0ff"|[[아치스 성단|아치스]]-F6
|<ref name=nelan>{{cite journal |last1=Nelan |first1=Edmund P. |last2=Walborn |first2=Nolan R. |last3=Wallace |first3=Debra J. |last4=Moffat |first4=Anthony F.J. |last5=Makidon |first5=Russell B. |last6=Gies |first6=Douglas R. |last7=Panagia |first7=Nino |date=July 2004 |title=Resolving OB systems in the Carina nebula with the Hubble Space Telescope Fine Guidance Sensor |journal=The Astronomical Journal |language=en |volume=128 |issue=1 |pages=323–329 |bibcode=2004AJ....128..323N |doi=10.1086/420716 |issn=0004-6256 |s2cid=121115585|doi-access=free }}</ref><ref name="ducati" />
|101–119
|- style="text-align:center;"
|-
| style="background: {{항성-색깔|O}};text-align:left;" | [[HSH95-36]] (in [[Tarantula Nebula]] of [[Large Magellanic Cloud|LMC]])
|bgcolor="#9bb0ff"|[[WR 102ka|작약성운 별]]<ref name="barniske">{{저널 인용
|110
| last1 = Barniske | first1 = A.
|163,000
| last2 = Oskinova | first2 = L. M.
|14.41
| last3 = Hamann | first3 = W. -R.
|49,500
| doi = 10.1051/0004-6361:200809568
|Evolution
| title = Two extremely luminous WN stars in the Galactic center with circumstellar emission from dust and gas
|{{SIMBAD link|HSH95+36|SIMBAD}}
| journal = Astronomy and Astrophysics
|<ref name="Brands2022" /><ref name=Doran2013/>
| volume = 486
|- style="text-align:center;"
| issue = 3
| style="background: {{항성-색깔|WC}};text-align:left;" | [[R146]] (in [[Tarantula Nebula]] of [[Large Magellanic Cloud|LMC]])
| pages = 971
|109
| year = 2008
|164,000
| pmid =
|13.11
| pmc =
|63,000
|arxiv = 0807.2476 |bibcode = 2008A&A...486..971B }}</ref>
|Spectroscopy
|{{SIMBAD link|RMC146|SIMBAD}}
|<ref name="hainich"/><ref name="Doran2013"/>
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[R136|R136a4]] (in [[Tarantula Nebula]] of [[Large Magellanic Cloud|LMC]])
|108
|157,000
|13.41
|50,000
|Evolution
|{{SIMBAD link|RMC136a4|SIMBAD}}
|<ref name="Brands2022" /><ref name=Doran2013/>
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[VFTS 621]] (in [[Tarantula Nebula]] of [[Large Magellanic Cloud|LMC]])
|107
|164,000
|15.39
|54,000
|Spectroscopy
|{{SIMBAD link|VFTS+621|SIMBAD}}
|<ref name="best"/><ref name=Doran2013/>
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[R136|R136a6]] (in [[Tarantula Nebula]] of [[Large Magellanic Cloud|LMC]])
|105
|157,000
|13.35
|52,000
|Evolution
|{{SIMBAD link|RMC136a6|SIMBAD}}
|<ref name="Brands2022" /><ref name=Doran2013/>
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[웨스터하우트 49]]-3 (in [[웨스터하우트 49]])
|105
|36,200
|16.689<br/>{{small|(J&nbsp;대역)}}
|40,700
|Evolution
|{{SIMBAD link|WBB2016+3|SIMBAD}}
|<ref name=Wu2016/><ref name=2MASS/>
|- style="text-align:center;"
| style="background: {{항성-색깔|WC}};text-align:left;" | [[WR 21a]] A ([[폭주성]] from [[웨스터룬드 2]])
|103.6
|26,100
|12.661 {{small|(연성계 전체)}}
|45,000
|Binary
|{{SIMBAD link|WR+21a|SIMBAD}}
|<ref name=tramper>{{Cite journal |last1=Tramper |first1=F. |last2=Sana |first2=H. |last3=Fitzsimons |first3=N.E. |last4=de Koter |first4=A. |last5=Kaper |first5=L. |last6=Mahy |first6=L. |last7=Moffat |first7=A. |date=11 January 2016 |title=The mass of the very massive binary WR21a |journal=Monthly Notices of the Royal Astronomical Society |language=en |volume=455 |issue=2 |pages=1275–1281 |arxiv=1510.03609 |bibcode=2016MNRAS.455.1275T |doi=10.1093/mnras/stv2373 |issn=0035-8711 |s2cid=44364798}}</ref><ref name="zacharias" />
|- style="text-align:center;"
| style="background: {{항성-색깔|WN}};text-align:left;" | [[R99]] (in [[N44 (emission nebula)|N44]] of [[Large Magellanic Cloud|LMC]])
|103
|164,000
|11.52
|28,000
|Spectroscopy
|{{SIMBAD link|RMC99|SIMBAD}}
|<ref name=hainich/><ref name=ducati/>
|- style="text-align:center;"
| style="background: {{항성-색깔|WC}};text-align:left;" | [[아치스 성단|아치스]]-F6 (WR 102ah in [[아치스 성단]])
|101
|25,000
|15.75<br/>{{small|(J&nbsp;대역)}}
|33,900
|Spectroscopy
|{{SIMBAD link|FNG2002+6|SIMBAD}}
|<ref name="grafener" /><ref name=Figer/>
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[Sk -65° 47]] (in [[NGC 1923]] of [[Large Magellanic Cloud|LMC]])
|101
|160,000
|12.466
|47,800
|Evolution
|{{SIMBAD link|Sk+-65+47|SIMBAD}}
|<ref name=Massey2000/><ref name=Bonanos/>
|- style="text-align:center;"
| style="background: {{항성-색깔|WC}};text-align:left;" |[[아치스 성단|아치스]]-F1 (WR 102ad in [[아치스 성단]])
|100.9
|25,000
|16.3<br/>{{small|(J&nbsp;대역)}}
|33,200
|Spectroscopy
|{{SIMBAD link|FNG2002+1|SIMBAD}}
|<ref name=grafener/><ref name=Figer/>
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[WR 102ka|Peony Star]] (WR 102ka in [[WR 102ka|Peony Nebula]] near [[Galactic Center]])
|100
|26,000
|12.978<br/>{{small|(J&nbsp;대역)}}
|25,100
|Spectroscopy
|{{SIMBAD link|Peony+Star|SIMBAD}}
|<ref name="oskinova">{{Cite journal|last1=Oskinova|first1=L. M.|last2=Steinke|first2=M.|last3=Hamann|first3=W.-R.|last4=Sander|first4=A.|last5=Todt|first5=H.|last6=Liermann|first6=A.|date=21 December 2013|title=One of the most massive stars in the Galaxy may have formed in isolation|journal=Monthly Notices of the Royal Astronomical Society|language=en|volume=436|issue=4|pages=3357–3365|arxiv=1309.7651|bibcode=2013MNRAS.436.3357O|doi=10.1093/mnras/stt1817|issn=0035-8711|s2cid=118513968}}</ref><ref name=2MASS/>
|- style="text-align:center;"
| style="background: {{항성-색깔|WC}};text-align:left;" | [[VFTS 457]] (in [[Tarantula Nebula]] of [[Large Magellanic Cloud|LMC]])
|100
|100
|164,000
|-
|13.74
|bgcolor="#9bb0ff"|성단 [[R136a]]
|39,800
|20개 이상 항성: 100
|Spectroscopy
|-
|{{SIMBAD link|VFTS+457|SIMBAD}}
|bgcolor="#aabfff"|[[HD 93129A|HD 93129 A]]
|<ref name="best"/><ref name=Doran2013/>
|- style="text-align:center;"
| style="background: {{항성-색깔|WN}};text-align:left;" | [[용골자리 에타]] A (in [[트럼플러 16]] of [[용골자리 성운]])
|100
|7,500
| style="background:lightblue;color:darkblue;" | '''4.3'''<br/>{{small|(연성계 전체)}}
|9,400–35,200
|Spectroscopy
|{{SIMBAD link|Eta+Carinae|SIMBAD}}
|<ref name="clementel">{{Cite journal|last1=Clementel |first1=N. |last2=Madura |first2=T.I. |last3=Kruip |first3=C.J.H. |last4=Paardekooper |first4=J.-P. |last5=Gull |first5=T.R. |date=1 March 2015 |title=3D radiative transfer simulations of Eta Carinae's inner colliding winds - I. Ionization structure of helium at apastron |journal=Monthly Notices of the Royal Astronomical Society |lang=en |volume=447 |issue=3 |pages=2445–2458 |arxiv=1412.7569 |bibcode=2015MNRAS.447.2445C|doi=10.1093/mnras/stu2614 |issn=0035-8711 |s2cid=118405692}}</ref><ref name="2018-07-02_NAL">{{cite journal |last1=Hamaguchi |first1=Kenji |last2=Corcoran |first2=Michael F. |last3=Pittard |first3=Julian M. |last4=Sharma |first4=Neetika |last5=Takahashi|first5=Hiromitsu|last6=Russell|first6=Christopher M.P. |last7=Grefenstette |first7=Brian W.|last8=Wik |first8=Daniel R.|last9=Gull |first9=Theodore R. |last10=Richardson |first10=Noel D. |last11=Madura |first11=Thomas I. |first12=Anthony F.J. |last12=Moffat |display-authors=6 |date=September 2018 |title=Non-thermal X-rays from colliding wind shock acceleration in the massive binary Eta Carinae |journal=Nature Astronomy |lang=en |volume=2 |issue=9 |pages=731–736 |arxiv=1904.09219 |bibcode=2018NatAs...2..731H |doi=10.1038/s41550-018-0505-1 |issn=2397-3366 |s2cid=126188024}}</ref>
|- style="text-align:center;"
| style="background: {{항성-색깔|WC}};text-align:left;" | [[머서 30]]-1 A (WR 46-3 A in [[머서 30]] of [[Dragonfish Nebula]])
|99
|40,000
|10.33<br/>{{small|(J&nbsp;대역)}}
|32,200
|Evolution
|{{SIMBAD link|DNB2016+Mc30-1|SIMBAD}}
|<ref name=Fuente>{{Cite journal |last1=de la Fuente |first1=D. |last2=Najarro |first2=F. |last3=Borissova |first3=J. |last4=Ramírez Alegría |first4=S. |last5=Hanson |first5=M.M. |last6=Trombley |first6=C. |last7=Figer |first7=D.F. |last8=Davies |first8=B. |last9=Garcia |first9=M. |last10=Kurtev|first10=R. |last11=Urbaneja |first11=M.A. |last12=Smith |first12=L.C. |last13=Lucas |first13=P.W. |last14=Herrero |first14=A. |display-authors=6 |date=May 2016 |title=Probing the Dragonfish star-forming complex: The ionizing population of the young massive cluster Mercer&nbsp;30 |journal=Astronomy & Astrophysics |volume=589 |page=A69 |arxiv=1602.02503 |bibcode=2016A&A...589A..69D |doi=10.1051/0004-6361/201528004 |issn=0004-6361 |s2cid=119096455}}</ref><ref group="lower-alpha" name=Mc30>Mercer&nbsp;30 is an open cluster in Dragonfish Nebula.</ref><ref name="Binary" group="lower-alpha" />
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[Sk -68° 137]] (in [[Tarantula Nebula]] of [[Large Magellanic Cloud|LMC]])
|99
|160,000
|13.346
|50,000
|Spectroscopy
|{{SIMBAD link|Sk+-68+137|SIMBAD}}
|<ref name="fulltext" /><ref name=Bonanos/>
|- style="text-align:center;"
| style="background: {{항성-색깔|WC}};text-align:left;" | [[WR 25]] A (in [[트럼플러 16]] of [[용골자리 성운]])
|98
|6,500
|8.8<br/>{{small|(연성계 전체)}}
|50,100
|Evolution
|{{SIMBAD link|WR+25|SIMBAD}}
|<ref name=hamann2019/><ref name=ducati/><ref group=lower-alpha name=Binary/>
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[BI 253]] ([[폭주성]] from [[Tarantula Nebula]] of [[Large Magellanic Cloud|LMC]])
|97.6
|164,000
|13.76
|54,000
|Spectroscopy
|{{SIMBAD link|BI+253|SIMBAD}}
|<ref name="schneider2018" /><ref>{{cite journal |last1=Rivero González |first1=J.G. |last2=Puls |first2=J. |last3=Najarro |first3=F. |last4=Brott |first4=I. |date=January 2012 |title=Nitrogen line spectroscopy of O-stars: II. Surface nitrogen abundances for O-stars in the Large Magellanic Cloud |journal=Astronomy & Astrophysics |volume=537 |page=A79 |arxiv=1110.5148 |bibcode=2012A&A...537A..79R |doi=10.1051/0004-6361/201117790 |issn=0004-6361 |s2cid=119110554}}</ref>
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[R136|R136a8]] (in [[Tarantula Nebula]] of [[Large Magellanic Cloud|LMC]])
|96
|157,000
|14.42
|49,500
|Evolution
|{{SIMBAD link|RMC136a8|SIMBAD}}
|<ref name="Brands2022" /><ref name=crowther2016>{{cite journal |last1=Crowther |first1=Paul A. |last2=Caballero-Nieves |first2=S.M. |last3=Bostroem |first3=K.A. |last4=Apellániz |first4=J. Maíz |last5=Schneider |first5=F.R.N. |last6=Walborn |first6=N.R. |last7=Angus |first7=C.R. |last8=Brott |first8=I. |last9=Bonanos |first9=A. |last10=de Koter |first10=A. |last11=de Mink |first11=S.E. |display-authors=6 |date=1 May 2016 |title=The R136 star cluster dissected with Hubble Space Telescope / STIS. I. Far-ultraviolet spectroscopic census and the origin of He{{sup{{sc|ii}}}} λ1640 in young star clusters |journal=Monthly Notices of the Royal Astronomical Society |language=en |volume=458 |issue=1 |pages=624–659 |arxiv=1603.04994 |bibcode=2016MNRAS.458..624C |doi=10.1093/mnras/stw273 |issn=0035-8711 |last12=Evans |first12=C.J. |last13=Gräfener |first13=G. |last14=Herrero |first14=A. |last15=Howarth |first15=I.D. |last16=Langer |first16=N. |last17=Lennon |first17=D.J. |last18=Puls |first18=J. |last19=Sana |first19=H. |last20=Vink |first20=J.S. |s2cid=119131482}}</ref>
|- style="text-align:center;"
| style="background: {{항성-색깔|WC}};text-align:left;" | [[HD 38282]] B (in [[Tarantula Nebula]] of [[Large Magellanic Cloud|LMC]])
|95
|95
|163,000
|-
|11.11<br/>{{small|(연성계 전체)}}
|bgcolor="#9bb0ff"|[[아치스 성단|아치스]]-F7
|47,000
|86–102
|Binary
|-
|{{SIMBAD link|HD+38282|SIMBAD}}
|bgcolor="#9bb0ff"|[[NGC 3603-A1]]b
|<ref name="sana">{{Cite journal |last1=Sana |first1=H. |last2=van Boeckel |first2=T. |last3=Tramper |first3=F. |last4=Ellerbroek |first4=L. E.|last5=de Koter |first5=A. |last6=Kaper |first6=L. |last7=Moffat|first7=A.F.J. |last8=Schnurr |first8=O. |last9=Schneider |first9=F.R.N. |last10=Gies |first10=D.R. |display-authors=6 |date=15 March 2013|title=R144 revealed as a double-lined spectroscopic binary|journal=Monthly Notices of the Royal Astronomical Society: Letters|language=en|volume=432|issue=1|pages=L26–L30|arxiv=1304.4591|bibcode=2013MNRAS.432L..26S|doi=10.1093/mnrasl/slt029|issn=1745-3933|s2cid=119238483}}</ref><ref name=zacharias/>
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[HM 1]]-6 (in [[HM 1]])
|95
|11,000
|11.64
|44,700
|Evolution
|{{SIMBAD link|Cl+HM+1+6|SIMBAD}}
|<ref name=Massey2001/><ref name=Reed>{{Cite journal|last=Reed|first=B. Cameron|date=May 2003|title=Catalog of Galactic OB Stars|journal=The Astronomical Journal|language=en|volume=125|issue=5|pages=2531–2533|bibcode=2003AJ....125.2531R|doi=10.1086/374771|issn=0004-6256|s2cid=121285799|doi-access=free}}</ref>
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[HD 97950|NGC 3603]]-42 (in [[HD 97950]] of [[NGC 3603]])
|95
|25,000
|12.86
|50,000
|Spectroscopy
|{{SIMBAD link|Cl*+NGC+3603+MDS+42|SIMBAD}}
|<ref name="fulltext" /><ref name=melena2008/>
|- style="text-align:center;"
| style="background: {{항성-색깔|WC}};text-align:left;" | [[R139]] A (in [[Tarantula Nebula]] of [[Large Magellanic Cloud|LMC]])
|95
|163,000
|11.94<br/>{{small|(연성계 전체)}}
|35,000
|Binary
|{{SIMBAD link|RMC139|SIMBAD}}
|<ref name="hainich" /><ref name=Doran2013/>
|- style="text-align:center;"
| style="background: {{항성-색깔|WC}};text-align:left;" | [[BAT99-6]] (in [[NGC 1747]] of [[Large Magellanic Cloud|LMC]])
|94
|165,000
|11.95
|56,000
|Spectroscopy
|{{SIMBAD link|BAT99+6|SIMBAD}}
|<ref name="hainich" /><ref name=Bonanos/>
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" |[[Sk -66° 172]] (in [[N64 (nebula)|N64]] of [[Large Magellanic Cloud|LMC]])
|94
|160,000
|13.1
|46,300
|Spectroscopy
|{{SIMBAD link|Sk+-66+172|SIMBAD}}
|<ref name="fulltext" /><ref name=Bonanos/><ref group="lower-alpha">N64 is an emission nebula in Large Magellanic Cloud.</ref>
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" |[[ST2-22]] (in [[NGC 2044]] of [[Large Magellanic Cloud|LMC]])
|94
|160,000
|14.3
|51,300
|Evolution
|{{SIMBAD link|ST92+2-22|SIMBAD}}
|<ref name=Massey2000/><ref name=Schild>{{Cite journal |last1=Schild |first1=H. |last2=Testor |first2=G. |date=March 1992 |title=Spectral types and UBV magnitudes of stars in the 30 Doradus complex |journal=Astronomy and Astrophysics Supplement Series |volume=92 |pages=729–748 |bibcode=1992A&AS...92..729S |issn=0365-0138 |s2cid=115371295}}</ref>
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" |[[VFTS 259]] (in [[Tarantula Nebula]] of [[Large Magellanic Cloud|LMC]])
|94
|164,000
|13.65
|37,600
|Spectroscopy
|{{SIMBAD link|VFTS+259|SIMBAD}}
|<ref name=best/><ref name=Doran2013/>
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[VFTS 562]] (in [[Tarantula Nebula]] of [[Large Magellanic Cloud|LMC]])
|94
|164,000
|13.66
|42,200
|Spectroscopy
|{{SIMBAD link|VFTS+562|SIMBAD}}
|<ref name="best" /><ref name=Doran2013/>
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[VFTS 512]] (in [[Tarantula Nebula]] of [[Large Magellanic Cloud|LMC]])
|93
|164,000
|14.28
|47,300
|Spectroscopy
|{{SIMBAD link|VFTS+512|SIMBAD}}
|<ref name="best" /><ref name=Doran2013/>
|- style="text-align:center;"
| style="background: {{항성-색깔|WC}};text-align:left;" | [[NGC 3603-A1|HD 97950 A1b]] (WR 43a B in [[HD 97950]] of [[NGC 3603]])
|92
|24,800
|11.18<br/>{{small|(연성계 전체)}}
|40,000
|Binary
|{{SIMBAD link|Cl*+NGC+3603+BLW+A1|SIMBAD}}
|<ref name="crowther" /><ref name=melena2008/>
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[R136b]] (in [[Tarantula Nebula]] of [[Large Magellanic Cloud|LMC]])
|92
|92
|163,000
|-
|13.24
|bgcolor="#cad8ff"|[[피스톨 별]]
|35,500
|86-92 또는 151
|Evolution
|-
|{{SIMBAD link|RMC136b|SIMBAD}}
|bgcolor="#aabfff"|[[아치스 성단|아치스]]-F15
|<ref name="Brands2022" /><ref name=Doran2013/>
|80–97
|- style="text-align:center;"
|-
| style="background: {{항성-색깔|O}};text-align:left;" | [[VFTS 16]] (in [[Tarantula Nebula]] of [[Large Magellanic Cloud|LMC]])
|bgcolor="#9bb0ff"|[[WR21a]]<ref>{{저널 인용
|91.6
| last1 = Niemela | first1 = V. S.
|164,000
| last2 = Gamen | first2 = R. C.
|13.55
| last3 = Barbá | first3 = R. H.
|50,600
| last4 = Fernández Lajús | first4 = E.
|Spectroscopy
| last5 = Benaglia | first5 = P.
|{{SIMBAD link|VFTS+16|SIMBAD}}
| last6 = Solivella | first6 = G. R.
|<ref name="schneider2018" /><ref name=Doran2013/>
| last7 = Reig | first7 = P.
|- style="text-align:center;"
| last8 = Coe | first8 = M. J.
| style="background: {{항성-색깔|O}};text-align:left;" | [[HD 97950]] A3 (in [[HD 97950]] of [[NGC 3603]])
| doi = 10.1111/j.1365-2966.2008.13684.x
|91
| title = The very massive X-ray bright binary system Wack 2134 (= WR 21a)
|24,800
| journal = Monthly Notices of the Royal Astronomical Society
|12.95
| volume = 389
|50,000
| issue = 3
|Spectroscopy
| pages = 1447
|{{SIMBAD link|Cl*+NGC+3603+BLW+A3|SIMBAD}}
| year = 2008
|<ref name="fulltext" /><ref name=melena2008/>
| pmid =
|- style="text-align:center;"
| pmc =
| style="background: {{항성-색깔|O}};text-align:left;" | [[NGC 346]]-W1 (in [[NGC 346]] of [[Small Magellanic Cloud|SMC]])
|arxiv = 0807.0728 |bibcode = 2008MNRAS.389.1447N }}</ref>
|91
|A=87, B=53
|200,000
|-
|12.57
|bgcolor="#9bb0ff"|[[웨스터룬드 2|WR20a]]
|43,400
|A=83, B=82
|Evolution
|-
|{{SIMBAD link|Cl*+NGC+346+W+1|SIMBAD}}
|bgcolor="#9bb0ff"|[[HD 38282]]
|<ref name=Massey2000/><ref name=spitzer>{{Cite journal |last1=Bonanos |first1=A.Z. |last2=Lennon |first2=D.J. |last3=Köhlinger |first3=F. |last4=van Loon |first4=J.Th. |last5=Massa |first5=D. L. |last6=Sewilo |first6=M. |last7=Evans|first7=C.J. |last8=Panagia |first8=N. |last9=Babler |first9=B.L. |last10=Block |first10=M. |last11=Bracker |first11=S. |last12=Engelbracht |first12=C.W. |last13=Gordon |first13=K.D. |last14=Hora |first14=J.L. |last15=Indebetouw |first15=R. |last16=Meade |first16=M.R. |last17=Meixner |first17=M.|last18=Misselt |first18=K.A. |last19=Robitaille |first19=T.P. |last20=Shiao |first20=B. |last21=Whitney |first21=B.A. |display-authors=6 |date=1 August 2010 |title=Spitzer SAGE-SMC infrared photometry of massive stars in the Small Magellanic Cloud |journal=[[The Astronomical Journal]] |volume=140 |issue=2 |pages=416–429 |arxiv=1004.0949 |bibcode=2010AJ....140..416B |doi=10.1088/0004-6256/140/2/416 |hdl=1887/61635 |issn=0004-6256 |s2cid=119290443}}</ref>
|>90 + >80
|- style="text-align:center;"
|-
| style="background:{{항성-색깔|O}};text-align:left;" |[[웨스터하우트 49-2]] (in [[웨스터하우트 49]])
|bgcolor="#aabfff"|[[Sk -71 51]]<ref name=meynadier>{{저널 인용
| 90–240, {{val|250|120}}
| doi = 10.1051/0004-6361:20042543
|36,200
| title = The LMC H II region N 214C and its peculiar nebular blob
|18.246<br/>{{small|(J&nbsp;대역)}}
| journal = Astronomy and Astrophysics
|35,500
| volume = 436
|Spectroscopy
| pages = 117
|{{SIMBAD link|WBB2016+2|SIMBAD}}
| year = 2005
|<ref name=Wu2016>{{Cite journal |last1=Wu |first1=Shi-Wei |last2=Bik |first2=Arjan |last3=Bestenlehner |first3=Joachim M. |last4=Henning |first4=Thomas |last5=Pasquali |first5=Anna |last6=Brandner |first6=Wolfgang |last7=Stolte |first7=Andrea |date=May 2016 |title=The massive stellar population of W49: A spectroscopic survey|journal=Astronomy & Astrophysics |volume=589 |page=A16 |arxiv=1602.05190 |bibcode=2016A&A...589A..16W|doi=10.1051/0004-6361/201527823|issn=0004-6361|s2cid=59425112}}</ref><ref name=2MASS>{{cite report |last1=Cutri |first1=Roc M. |last2=Skrutskie |first2=Michael F. |last3=van&nbsp;Dyk |first3=Schuyler D. |last4=Beichman |first4=Charles A. |last5=Carpenter |first5=John M. |last6=Chester |first6=Thomas |last7=Cambresy |first7=Laurent |last8=Evans |first8=Tracey E. |last9=Fowler |first9=John W. |last10=Gizis |first10=John E. |last11=Howard |first11=Elizabeth V. |last12=Huchra |first12=John P. |last13=Jarrett |first13=Thomas H. |last14=Kopan |first14=Eugene L. |last15=Kirkpatrick |first15=J. Davy |last16=Light |first16=Robert M. |last17=Marsh |first17=Kenneth A. |last18=McCallon |first18=Howard L. |last19=Schneider |first19=Stephen E. |last20=Stiening |first20=Rae |last21=Sykes |first21=Matthew J. |last22=Weinberg |first22=Martin D. |last23=Wheaton |first23=William A. |last24=Wheelock |first24=Sherry L. |last25=Zacarias |first25=N. |display-authors=6 |year=2003 |title=VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003) |publisher=CDS/ADC |series=Collection of Electronic Catalogues |bibcode=2003yCat.2246....0C |page=II/246 |volume=2246 |url=http://vizier.u-strasbg.fr/viz-bin/VizieR?-source=II/246 |s2cid=115529446}}</ref>
| last1 = Meynadier | first1 = F.
|- style="text-align:center;"
| last2 = Heydari-Malayeri | first2 = M.
| style="background: {{항성-색깔|WN}};text-align:left;" | [[R127]] (in [[NGC 2055]] of [[Large Magellanic Cloud|LMC]])
| last3 = Walborn | first3 = N. R.
|90
}}</ref>
|160,000
|10.15
|10,000–27,000
|Evolution
|{{SIMBAD link|RMC127|SIMBAD}}
|<ref name=Smith2015>{{cite journal |last1=Smith |first1=Nathan |last2=Tombleson |first2=Ryan |date=11 February 2015 |title=Luminous blue variables are antisocial: their isolation implies that they are kicked mass gainers in binary evolution |journal=[[Monthly Notices of the Royal Astronomical Society]] |lang=en |volume=447 |issue=1 |pages=598–617 |arxiv=1406.7431 |bibcode=2015MNRAS.447..598S |doi=10.1093/mnras/stu2430 |issn=1365-2966 |s2cid=119284620}}</ref><ref name=zacharias/>
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[VFTS 333]] (in [[Tarantula Nebula]] of [[Large Magellanic Cloud|LMC]])
|90
|164,000
|12.49
|37,600
|Spectroscopy
|{{SIMBAD link|VFTS+333|SIMBAD}}
|<ref name=best/><ref name=Doran2013/>
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[VFTS 267]] (in [[타란툴라 성운] of [[Large Magellanic Cloud|LMC]])
|89
|164,000
|13.49
|44,700
|Spectroscopy
|{{SIMBAD link|VFTS+267|SIMBAD}}
|<ref name="best" /><ref name="Doran2013" />
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[VFTS 64]] (in [[타란툴라 성운]] of [[Large Magellanic Cloud|LMC]])
|88
|164,000
|14.621
|39,800
|Spectroscopy
|{{SIMBAD link|VFTS+64|SIMBAD}}
|<ref name=best/><ref name=Bonanos/>
|- style="text-align:center;"
| style="background: {{항성-색깔|WC}};text-align:left;" | [[BAT99-80]] A (in [[NGC 2044]] of [[Large Magellanic Cloud|LMC]])
|87
|165,000
|13<br/>{{small|(연성계 전체)}}
|45,000
|Spectroscopy
|{{SIMBAD link|BAT99+80|SIMBAD}}
|<ref name=Massey2000/><ref name=Schild/>
|- style="text-align:center;"
| style="background: {{항성-색깔|WC}};text-align:left;" | [[R140b]] (in [[타란툴라 성운]] of [[Large Magellanic Cloud|LMC]])
|87
|165,000
|12.66
|47,000
|Spectroscopy
|{{SIMBAD link|RMC140b|SIMBAD}}
|<ref name=hainich/><ref name=Doran2013/>
|- style="text-align:center;"
| style="background: {{항성-색깔|WC}};text-align:left;" | [[VFTS 542]] (in [[타란툴라 성운]] of [[Large Magellanic Cloud|LMC]])
|87
|164,000
|13.47
|44,700
|Spectroscopy
|{{SIMBAD link|VFTS+542|SIMBAD}}
|<ref name="best" /><ref name=Doran2013/>
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[VFTS 599]] (in [[타란툴라 성운]] of [[Large Magellanic Cloud|LMC]])
|87
|164,000
|13.8
|44,700
|Spectroscopy
|{{SIMBAD link|VFTS+599|SIMBAD}}
|<ref name="best" /><ref name="Doran2013" />
|- style="text-align:center;"
| style="background: {{항성-색깔|WC}};text-align:left;" | [[WR 89]] (in [[HM 1]])
|87
|11,000
|11.02
|39,800
|Evolution
|{{SIMBAD link|WR+89|SIMBAD}}
|<ref name=hamann2019/><ref name=zacharias/>
|- style="text-align:center;"
| style="background: {{항성-색깔|WC}};text-align:left;" | [[아치스 성단|아치스]]-F7 (WR 102aj in [[아치스 성단]])
|86.3
|25,000
|15.74<br/>{{small|(J&nbsp;대역)}}
|32,900
|Spectroscopy
|{{SIMBAD link|FNG2002+7|SIMBAD}}
|<ref name=grafener/><ref name=Figer/>
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[Sk -69° 104]] (in [[NGC 1910]] of [[Large Magellanic Cloud|LMC]])
|86
|160,000
|12.1
|39,900
|Evolution
|{{SIMBAD link|Sk+-69+104|SIMBAD}}
|<ref name=Massey2000/><ref name=Bonanos/>
|- style="text-align:center;"
| style="background: {{항성-색깔|WC}};text-align:left;" | [[VFTS 1017]] (in [[타란툴라 성운]] of [[Large Magellanic Cloud|LMC]])
|86
|164,000
|14.5
|50,100
|Spectroscopy
|{{SIMBAD link|VFTS+1017|SIMBAD}}
|<ref name="best" /><ref name="Doran2013" />
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[LH 10]]-3061 (in [[NGC 1763]] of [[Large Magellanic Cloud|LMC]])
|85
|160,000
|13.491
|52,000
|Spectroscopy
|{{SIMBAD link|L72+LH+10-3061|SIMBAD}}
|<ref name="fulltext" /><ref name=Bonanos/>
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[NGC 346|Sk 80]] (in [[NGC 346]] of [[Small Magellanic Cloud|SMC]])
|85
|200,000
|12.31
|38,900
|Evolution
|{{SIMBAD link|Sk+80|SIMBAD}}
|<ref name=Massey2000/><ref>{{cite journal |last1=Evans |first1=C.J. |last2=Lennon |first2=D.J. |last3=Smartt |first3=S. J. |last4=Trundle |first4=C. |date=September 2006 |title=The VLT-FLAMES survey of massive stars: observations centered on the Magellanic Cloud clusters NGC 330, NGC 346, NGC 2004, and the N11 region |journal=[[Astronomy & Astrophysics]] |volume=456 |issue=2 |pages=623–638 |arxiv=astro-ph/0606405 |bibcode=2006A&A...456..623E |doi=10.1051/0004-6361:20064988 |issn=0004-6361 |s2cid=13160849}}</ref>
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[VFTS 603]] (in [[타란툴라 성운]] of [[Large Magellanic Cloud|LMC]])
|85
|164,000
|13.99
|42,200
|Spectroscopy
|{{SIMBAD link|VFTS+603|SIMBAD}}
|<ref name=best/><ref name=Doran2013/>
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[Sk -70° 91]] (in [[BSDL 1830]] of [[Large Magellanic Cloud|LMC]])
|84.09
|165,000
|12.78
|48,900
|Evolution
|{{SIMBAD link|Sk+-70+91|SIMBAD}}
|<ref name=Massa2017>{{Cite journal|last1=Massa|first1=D.|last2=Fullerton|first2=A. W.|last3=Prinja|first3=R. K.|date=September 2017|title=Mass-loss rates from mid-infrared excesses in LMC and SMC O stars|journal=Monthly Notices of the Royal Astronomical Society|language=en|volume=470|issue=3|pages=3765–3774|arxiv=1706.02627|bibcode=2017MNRAS.470.3765M|doi=10.1093/mnras/stx1443|issn=0035-8711|s2cid=119475951}}</ref><ref name=Bonanos/><ref group="lower-alpha">BSDL 1830 is a star cluster in Large Magellanic Cloud.</ref>
|- style="text-align:center;"
| style="background: {{항성-색깔|WC}};text-align:left;" | [[R147]] (in [[타란툴라 성운]] of [[Large Magellanic Cloud|LMC]])
|84
|164,000
|12.993
|47,300
|Spectroscopy
|{{SIMBAD link|RMC147|SIMBAD}}
|<ref name=best/><ref name=Ulaczyk/>
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[HD 93250]] A (in [[트럼플러 16]] of [[용골자리 성운]])
|83.3
|7,500
|7.5<br/>{{small|(연성계 전체)}}
|46,000
|Evolution
|{{SIMBAD link|HD+93250|SIMBAD}}
|<ref name=weidner>{{Cite journal |last1=Weidner |first1=C. |last2=Vink |first2=J.S. |date=December 2010 |title=The masses, and the mass discrepancy of O-type stars |journal=[[Astronomy & Astrophysics]] |volume=524 |page=A98 |arxiv=1010.2204 |bibcode=2010A&A...524A..98W |doi=10.1051/0004-6361/201014491 |issn=0004-6361 |s2cid=118836634}}</ref><ref name=ducati/><ref group=lower-alpha name=Binary/>
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[멜닉 33Na]] A (in [[타란툴라 성운]] of [[Large Magellanic Cloud|LMC]])
|83
|163,000
|13.79<br/>{{small|(연성계 전체)}}
|50,000
|Evolution
|{{SIMBAD link|Cl*+NGC+2070+MEL+33N|SIMBAD}}
|<ref name=Bestenlehner2022>{{cite journal|doi=10.1093/mnras/stab3521|title=Melnick 33Na: A very massive colliding-wind binary system in 30 Doradus|year=2022|last1=Bestenlehner|first1=Joachim M.|last2=Crowther|first2=Paul A.|last3=Broos|first3=Patrick S.|last4=Pollock|first4=Andrew M T.|last5=Townsley|first5=Leisa K.|journal=Monthly Notices of the Royal Astronomical Society|volume=510|issue=4|pages=6133–6149|bibcode=2022MNRAS.510.6133B|arxiv=2112.00022}}</ref><ref name=Castro2018>{{cite journal|doi=10.1051/0004-6361/201732084|title=Mapping the core of the Tarantula Nebula with VLT-MUSE. I. Spectral and nebular content around R136|year=2018 |author1=Castro, N. |author2=Crowther, P. A. |author3=Evans, C.J. |author4=Mackey, J. |author5=Castro-Rodriguez, N. |author6=Vink, J.S. |author7=Melnick, J. |author8=Selman, F. |display-authors=6 |journal=[[Astronomy & Astrophysics]] |volume=614 |id=A147 |page=12 |arxiv=1802.01597 |bibcode=2018A&A...614A.147C |s2cid=119341920}}</ref>
|- style="text-align:center;"
| style="background: {{항성-색깔|WC}};text-align:left;" | [[WR 20a]] A (in [[웨스터룬드 2]])
|82.7
|20,000
|13.28<br/>{{small|(연성계 전체)}}
|43,000
|Binary
|{{SIMBAD link|WR+20a|SIMBAD}}
|<ref name="rauw">{{cite journal |last1=Rauw |first1=G. |last2=Crowther |first2=P.A. |last3=de Becker |first3=M. |last4=Gosset |first4=E. |last5=Nazé |first5=Y. |last6=Sana |first6=H. |last7=van der Hucht |first7=K.A. |last8=Vreux |first8=J.-M. |last9=Williams |first9=P.M. |display-authors=6 |date=March 2005 |title=The spectrum of the very massive binary system WR 20a (WN6ha + WN6ha): Fundamental parameters and wind interactions |journal=Astronomy & Astrophysics |volume=432 |issue=3 |pages=985–998 |bibcode=2005A&A...432..985R |doi=10.1051/0004-6361:20042136 |doi-access=free |issn=0004-6361 |s2cid=53372849}}</ref>
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[TIC 276934932]] A (in [[NGC 2048]] of [[Large Magellanic Cloud|LMC]])
|82
|160,000
|14.05<br/>{{small|(연성계 전체)}}
|45,000
|Spectroscopy
|{{SIMBAD link|TIC+276934932|SIMBAD}}
|<ref name="fulltext"/><ref name=Bonanos/>
|- style="text-align:center;"
| style="background: {{항성-색깔|WC}};text-align:left;" | [[WR 20a]] B (in [[웨스터룬드 2]])
|81.9
|20,000
|13.28<br/>{{small|(연성계 전체)}}
|43,000
|Binary
|{{SIMBAD link|WR+20a|SIMBAD}}
|<ref name="rauw" />
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[트럼플러 27]]-27 (in [[트럼플러 27]])
|81
|3,900
|13.31
|37,000
|Evolution
|{{SIMBAD link|Cl+Trumpler+27+27|SIMBAD}}
|<ref name=Massey2001/><ref name=zacharias/>
|- style="text-align:center;"
| style="background: {{항성-색깔|WC}};text-align:left;" | [[BAT99-96]] (in [[Tarantula Nebula]] of [[Large Magellanic Cloud|LMC]])
|80
|80
|165,000
|-
|13.76
|bgcolor="#aabfff"|[[백조자리 OB2]]-8B
|42,000
|Spectroscopy
|{{SIMBAD link|BAT99+96|SIMBAD}}
|<ref name=hainich/><ref name=Doran2013/>
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[HD 15570]] (in [[IC 1805]] of [[Heart Nebula]])
|80
|80
|7,500
|-
|8.11
|bgcolor="#aabfff"|[[R139]]<ref>{{저널 인용
|46,000
| last1 = Taylor | first1 = W. D.
|Spectroscopy
| last2 = Evans | first2 = C. J.
|{{SIMBAD link|HD+15570|SIMBAD}}
| last3 = Sana | first3 = H.
|<ref name=debecker/><ref name=ducati/>
| last4 = Walborn | first4 = N. R.
|- style="text-align:center;"
| last5 = De Mink | first5 = S. E.
| style="background: {{항성-색깔|WC}};text-align:left;" | [[HD 38282]] A (in [[Tarantula Nebula]] of [[Large Magellanic Cloud|LMC]])
| last6 = Stroud | first6 = V. E.
|80
| last7 = Alvarez-Candal | first7 = A.
|163,000
| last8 = Barbá | first8 = R. H.
|11.11<br/>{{small|(연성계 전체)}}
| last9 = Bestenlehner | first9 = J. M.
|47,000
| last10 = Bonanos | first10 = A. Z.
|Binary
| last11 = Brott | first11 = I.
|{{SIMBAD link|HD+38282|SIMBAD}}
| last12 = Crowther | first12 = P. A.
|<ref name=sana/><ref name=zacharias/>
| last13 = De Koter | first13 = A.
|- style="text-align:center;"
| last14 = Friedrich | first14 = K.
| style="background: {{항성-색깔|O}};text-align:left;" | [[HSH95-46]] (in [[Tarantula Nebula]] of [[Large Magellanic Cloud|LMC]])
| last15 = Gräfener | first15 = G.
|80
| last16 = Hénault-Brunet | first16 = V.
|163,000
| last17 = Herrero | first17 = A.
|14.56
| last18 = Kaper | first18 = L.
|47,500
| last19 = Langer | first19 = N.
|Evolution
| last20 = Lennon | first20 = D. J.
|{{SIMBAD link|HSH95+46|SIMBAD}}
| last21 = Maíz Apellániz | first21 = J.
|<ref name=Brands2022/><ref name=Doran2013/>
| last22 = Markova | first22 = N.
|- style="text-align:center;"
| last23 = Morrell | first23 = N.
| style="background: {{항성-색깔|O}};text-align:left;" | [[아치스 성단|아치스]]-F15 (in [[아치스 성단]])
| last24 = Monaco | first24 = L.
|79.7
| last25 = Vink | first25 = J. S.
|25,000
| title = The VLT-FLAMES Tarantula Survey
|16.12<br/>{{small|(J&nbsp;대역)}}
| doi = 10.1051/0004-6361/201116785
|35,600
| journal = Astronomy & Astrophysics
|Spectroscopy
| volume = 530
|{{SIMBAD link|FNG2002+15|SIMBAD}}
| pages = L10
|<ref name=grafener/><ref name=Figer/>
| year = 2011
|- style="text-align:center;"
| pmid =
| style="background: {{항성-색깔|O}};text-align:left;" | [[BI 237]] (in [[BSDL 2527]] of [[Large Magellanic Cloud|LMC]])
| pmc =
|79.66
|arxiv = 1103.5387 |bibcode = 2011A&A...530L..10T }}</ref>
|165,000
|A=78, B=66
|13.83
|-
|51,300
|bgcolor="#9bb0ff"|[[용골자리 V429]] A + B
|Spectroscopy
|A=78, B=21
|{{SIMBAD link|BI+237|SIMBAD}}
|-
|<ref name=Massa2017/><ref name=Bonanos/><ref group="lower-alpha">BSDL 2527 is a star cluster in Large Magellanic Cloud.</ref>
|bgcolor="#9bb0ff"|[[WR 22]]
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[VFTS 94]] (in [[Tarantula Nebula]] of [[Large Magellanic Cloud|LMC]])
|79
|164,000
|14.161
|42,200
|Spectroscopy
|{{SIMBAD link|VFTS+94|SIMBAD}}
|<ref name="best" /><ref name=Bonanos/>
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[VFTS 151]] (in [[Tarantula Nebula]] of [[Large Magellanic Cloud|LMC]])
|79
|164,000
|14.13
|42,200
|Spectroscopy
|{{SIMBAD link|VFTS+151|SIMBAD}}
|<ref name="best" /><ref name="Doran2013" />
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[LH 41]]-32 (in [[NGC 1910]] of [[Large Magellanic Cloud|LMC]])
|78
|78
|160,000
|-
|13.086
|bgcolor="#aabfff"|[[피스미스 24|피스미스 24-17]]<ref>{{저널 인용
|48,200
| last1 = Fang | first1 = M.
|Evolution
| last2 = Van Boekel | first2 = R.
|{{SIMBAD link|L72+LH+41-32|SIMBAD}}
| last3 = King | first3 = R. R.
|<ref name=Massey2000/><ref name=Bonanos/>
| last4 = Henning | first4 = T.
|- style="text-align:center;"
| last5 = Bouwman | first5 = J.
| style="background: {{항성-색깔|O}};text-align:left;" | [[피스미스 24]]-17 (in [[피스미스 24]] of [[NGC 6357]])
| last6 = Doi | first6 = Y.
|78
| last7 = Okamoto | first7 = Y. K.
|5,900
| last8 = Roccatagliata | first8 = V.
|11.84
| last9 = Sicilia-Aguilar | first9 = A.
|42,700
| title = Star formation and disk properties in Pismis 24
|Spectroscopy
| doi = 10.1051/0004-6361/201015914
|{{SIMBAD link|Cl+Pismis+24+17|SIMBAD}}
| journal = Astronomy & Astrophysics
|<ref name="fang">{{Cite journal|last1=Fang|first1=M.|last2=van Boekel|first2=R.|last3=King|first3=R. R.|last4=Henning|first4=Th.|last5=Bouwman|first5=J.|last6=Doi|first6=Y.|last7=Okamoto|first7=Y. K.|last8=Roccatagliata|first8=V.|last9=Sicilia-Aguilar|first9=A. |display-authors=6 |date=March 2012|title=Star formation and disk properties in Pismis 24|journal=Astronomy & Astrophysics|volume=539|page=A119|arxiv=1201.0833|bibcode=2012A&A...539A.119F|doi=10.1051/0004-6361/201015914|issn=0004-6361|s2cid=73612793}}</ref><ref name=Reed/>
| volume = 539
|- style="text-align:center;"
| pages = A119
| style="background: {{항성-색깔|O}};text-align:left;" | [[VFTS 404]] (in [[Tarantula Nebula]] of [[Large Magellanic Cloud|LMC]])
| year = 2012
| pmid =
| pmc =
|arxiv = 1201.0833 |bibcode = 2012A&A...539A.119F }}</ref>
|78
|78
|164,000
|-
|14.14
|bgcolor="#9bb0ff"|[[아치스 성단|아치스]]-F12
|44,700
|70–82
|Spectroscopy
|-
|{{SIMBAD link|VFTS+404|SIMBAD}}
|bgcolor="#aabfff"|[[백조자리 OB2]]-10
|<ref name=best/><ref name=Doran2013/>
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[웨스터하우트 51]]-2 (in [[웨스터하우트 51]])
|77
|20,000
|13.68<br/>{{small|(J&nbsp;대역)}}
|42,700
|Evolution
|{{SIMBAD link|2MASS+J19230169%2B1416403|SIMBAD}}
|<ref name=Bik/>
|- style="text-align:center;"
| style="background: {{항성-색깔|WC}};text-align:left;" | [[BAT99-68]] (in [[BSDL 2505]] of [[Large Magellanic Cloud|LMC]])
|76
|165,000
|14.13
|45,000
|Spectroscopy
|{{SIMBAD link|BAT99+68|SIMBAD}}
|<ref name="hainich" /><ref name=Bonanos/><ref group="lower-alpha">BSDL 2505 is a star cluster in Large Magellanic Cloud.</ref>
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[콜린더 228|HD 93632]] (in [[콜린더 228]] of [[용골자리 성운]])
|76
|10,000
|8.23
|45,400
|Evolution
|{{SIMBAD link|HD+93632|SIMBAD}}
|<ref name=Massey2001/><ref name="ducati" />
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[NGC 346]]-W3 (in [[NGC 346]] of [[Small Magellanic Cloud|SMC]])
|76
|200,000
|12.8
|52,500
|Evolution
|{{SIMBAD link|Cl*+NGC+346+W+3|SIMBAD}}
|<ref name=Massey2000/><ref name="spitzer" />
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[VFTS 169]] (in [[Tarantula Nebula]] of [[Large Magellanic Cloud|LMC]])
|76
|164,000
|14.437
|47,300
|Spectroscopy
|{{SIMBAD link|VFTS+169|SIMBAD}}
|<ref name="best" /><ref name=Bonanos/>
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[VFTS 440]] (in [[Tarantula Nebula]] of [[Large Magellanic Cloud|LMC]])
|76
|164,000
|12.046
|39,800
|Spectroscopy
|{{SIMBAD link|VFTS+440|SIMBAD}}
|<ref name="best" /><ref name=Bonanos/>
|- style="text-align:center;"
| style="background: {{항성-색깔|WC}};text-align:left;" | [[AB1 (항성)|AB1]] (in [[DEM S10]] of [[Small Magellanic Cloud|SMC]])
|75
|75
|197,000
|-
|15.238
|bgcolor="#aabfff"|[[아치스 성단|아치스]]-F18
|79,000
|67–82
|Spectroscopy
|-
|{{SIMBAD link|SMC+AB+1|SIMBAD}}
|bgcolor="#fbf8ff"|[[메시에 33|M33]] 내 [[Var 83]]
|<ref name=Hainich2015>{{Cite journal|last1=Hainich|first1=R.|last2=Pasemann|first2=D.|last3=Todt|first3=H.|last4=Shenar|first4=T.|last5=Sander|first5=A.|last6=Hamann|first6=W. -R|date=2015|title=Wolf-Rayet stars in the Small Magellanic Cloud. I. Analysis of the single WN stars|journal=Astronomy & Astrophysics|volume=581|issue=21|page=30|arxiv=1507.04000|bibcode=2015A&A...581A..21H|doi=10.1051/0004-6361/201526241|s2cid=56230998}}</ref><ref name="spitzer" /><ref group="lower-alpha">DEM S10 is a H II region in Small Magellanic Cloud.</ref>
|60–85
|- style="text-align:center;"
|-
| style="background: {{항성-색깔|WC}};text-align:left;" | [[WR 22]] A (in [[Bochum 10]] of [[용골자리 성운]])
|bgcolor="#aabfff"|[[백조자리 OB2]]-8C
|75
|8,300
| style="background:lightblue;color:darkblue;" |'''6.42'''<br/>{{small|(연성계 전체)}}
|44,700
|Evolution
|{{SIMBAD link|WR+22|SIMBAD}}
|<ref name="hamann2019" /><ref name="ducati" /><ref group="lower-alpha" name="WR22">Bochum 10 is an open cluster in Carina Nebula.</ref>
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[피스미스 24-1]]NE (in [[피스미스 24]] of [[NGC 6357]])
|74
|6,500
|11
|42,500
|Binary
|{{SIMBAD link|CL+PISMIS+24-1NE|SIMBAD}}
|<ref name="fang" /><ref name="skiff">{{Cite journal|last1=Skiff|first1=B. A.|date=October 2014|title=VizieR Online Data Catalog: Catalogue of Stellar Spectral Classifications (Skiff, 2009- )|journal=VizieR On-Line Data Catalog: B/Mk. Originally Published in: Lowell Observatory (October 2014)|volume=1|bibcode=2014yCat....1.2023S|s2cid=215961366}}</ref>
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[VFTS 608]] (in [[Tarantula Nebula]] of [[Large Magellanic Cloud|LMC]])
|74
|164,000
|14.22
|42,200
|Spectroscopy
|{{SIMBAD link|VFTS+608|SIMBAD}}
|<ref name="best" /><ref name="Doran2013" />
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[HSH95-31]] (in [[Tarantula Nebula]] of [[Large Magellanic Cloud|LMC]])
|73
|163,000
|14.12
|47,500
|Evolution
|{{SIMBAD link|HSH95+31|SIMBAD}}
|<ref name=Brands2022/><ref name=Doran2013/>
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[머서 30]]-3 (in [[머서 30]] of [[Dragonfish Nebula]])
|73
|40,000
|12.62<br/>{{small|(J&nbsp;대역)}}
|39,300
|Evolution
|{{SIMBAD link|DNB2016+Mc30-3|SIMBAD}}
|<ref name=Fuente/><ref group=lower-alpha name=Mc30/>
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[머서 30]]-11 (in [[머서 30]] of [[Dragonfish Nebula]])
|73
|40,000
|12.33<br/>{{small|(J&nbsp;대역)}}
|36,800
|Evolution
|{{SIMBAD link|DNB2016+Mc30-11|SIMBAD}}
|<ref name=Fuente/><ref group=lower-alpha name=Mc30/>
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[VFTS 566]] (in [[Tarantula Nebula]] of [[Large Magellanic Cloud|LMC]])
|73
|164,000
|14.05
|44,700
|Spectroscopy
|{{SIMBAD link|VFTS+566|SIMBAD}}
|<ref name="best" /><ref name="Doran2013" />
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[LH 64]]-16 (in [[NGC 2001]] of [[Large Magellanic Cloud|LMC]])
|72
|160,000
|13.666
|50,900
|Evolution
|{{SIMBAD link|L72+LH+64-16|SIMBAD}}
|<ref name=Massey2000/><ref name="Zaritsky" />
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[NGC 2044]]-W35 (in [[NGC 2044]] of [[Large Magellanic Cloud|LMC]])
|72
|160,000
|14.1
|48,200
|Evolution
|{{SIMBAD link|WDP99+NGC+2044W+35|SIMBAD}}
|<ref name=Massey2000/><ref name=Bonanos/>
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[VFTS 216]] (in [[Tarantula Nebula]] of [[Large Magellanic Cloud|LMC]])
|72
|164,000
|14.389
|44,700
|Spectroscopy
|{{SIMBAD link|VFTS+216|SIMBAD}}
|<ref name="best" /><ref name=Bonanos/>
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[ST2-1]] (in [[NGC 2044]] of [[Large Magellanic Cloud|LMC]])
|71
|71
|160,000
|-
|14.3
|bgcolor="#9bb0ff"|[[아치스 성단|아치스]]-F4
|44,100
|66–76
|Evolution
|-
|{{SIMBAD link|ST92+2-1|SIMBAD}}
|bgcolor="#aabfff"|[[R126]]
|<ref name=Massey2000/><ref name="Schild" />
|- style="text-align:center;"
| style="background: {{항성-색깔|B}};text-align:left;" | [[VFTS 3]] (in [[타란툴라 성운]] of [[Large Magellanic Cloud|LMC]])
|71
|164,000
|11.56
|21,000
|Spectroscopy
|{{SIMBAD link|VFTS+3|SIMBAD}}
|<ref name=McEvoy>{{Cite journal |last1=McEvoy |first1=C.M. |last2=Dufton |first2=P.L. |last3=Evans |first3=C.J. |last4=Kalari |first4=V.M. |last5=Markova |first5=N.|last6=Simón-Díaz |first6=S. |last7=Vink|first7=J.S. |last8=Walborn |first8=N.R. |last9=Crowther |first9=P.A. |last10=de Koter |first10=A. |last11=de Mink |first11=S.E. |last12=Dunstall |first12=P.R. |last13=Hénault-Brunet |first13=V. |last14=Herrero |first14=A. |last15=Langer |first15=N. |last16=Lennon |first16=D. J.|last17=Maíz Apellániz |first17=J. |last18=Najarro |first18=F. |last19=Puls |first19=J. |last20=Sana|first20=H. |last21=Schneider |first21=F.R.N. |last22=Taylor|first22=W.D. |display-authors=6 |date=March 2015|title=The VLT-FLAMES Tarantula Survey: XIX. B-type supergiants: Atmospheric parameters and nitrogen abundances to investigate the role of binarity and the width of the main sequence⋆|journal=Astronomy & Astrophysics|volume=575|page=A70|doi=10.1051/0004-6361/201425202|issn=0004-6361|arxiv=1412.2705|bibcode=2015A&A...575A..70M|s2cid=39125418}}</ref><ref name="Doran2013" />
|- style="text-align:center;"
| style="background: {{항성-색깔|WC}};text-align:left;" | [[아치스 성단|아치스]]-F12 (WR 102af in [[아치스 성단]])
|70
|70
|25,000
|-
|16.4<br/>{{small|(J&nbsp;대역)}}
|bgcolor="#aabfff"|[[M33 X-7]]의 짝별<ref>{{저널 인용
|36,900
| last1 = Orosz | first1 = J. A.
|Spectroscopy
| last2 = McClintock | first2 = J. E.
|{{SIMBAD link|FNG2002+12|SIMBAD}}
| last3 = Narayan | first3 = R.
|<ref name=grafener/><ref name=Figer/>
| last4 = Bailyn | first4 = C. D.
|- style="text-align:center;"
| last5 = Hartman | first5 = J. D.
| style="background: {{항성-색깔|O}};text-align:left;" | [[HD 15629]] (in [[IC 1805]] of [[Heart Nebula]])
| last6 = Macri | first6 = L.
| last7 = Liu | first7 = J.
| last8 = Pietsch | first8 = W.
| last9 = Remillard | first9 = R. A.
| last10 = Shporer
| doi = 10.1038/nature06218 | first10 = A.
| last11 = Mazeh | first11 = T.
| title = A 15.65-solar-mass black hole in an eclipsing binary in the nearby spiral galaxy M 33
| journal = Nature
| volume = 449
| issue = 7164
| pages = 872–875
| year = 2007
| pmid = 17943124
| pmc =
}}</ref>
|70
|70
|7,500
|-
|8.42
|bgcolor="#fbf8ff"|[[용골자리 AG]]
|45,900
|Spectroscopy
|{{SIMBAD link|HD+15629|SIMBAD}}
|<ref name=debecker/><ref name=ducati/>
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[HD 37974]] (in [[N135]] of [[Large Magellanic Cloud|LMC]])
|70
|70
|163,000
|-
|10.99
|bgcolor="#aabfff"|[[BD+43° 3654]]
|22,500
|Spectroscopy
|{{SIMBAD link|HD+37974|SIMBAD}}
|<ref name="kastner">{{Cite journal|last1=Kastner|first1=Joel H.|last2=Buchanan|first2=Catherine L.|last3=Sargent|first3=B.|last4=Forrest|first4=W. J.|date=10 February 2006|title=Spitzer Spectroscopy of Dusty Disks around B[e] Hypergiants in the Large Magellanic Cloud|journal=The Astrophysical Journal|language=en|volume=638|issue=1|pages=L29–L32|bibcode=2006ApJ...638L..29K|doi=10.1086/500804|issn=0004-637X|s2cid=121769413|doi-access=free}}</ref><ref name="zacharias" /><ref group="lower-alpha">N135 is an emission nebula in Large Magellanic Cloud.</ref>
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[HD 93129]] Ab (in [[트럼플러 14]] of [[용골자리 성운]])
|70
|70
|7,500
|-
|7.31<br/>{{small|(연성계 전체)}}
|bgcolor="#9bb0ff"|[[HD 5980]] A + B
|44,000
|A=58-79, B=51-67
|Trinary
|-
|{{SIMBAD link|HD+93129A|SIMBAD}}
|bgcolor="#aabfff"|[[피스미스 24-1]] SW
|<ref name="nelan" /><ref name=tycho2>{{Cite journal |last1=Høg |first1=E. |last2=Fabricius |first2=C. |last3=Makarov |first3=V.V. |last4=Urban |first4=S. |last5=Corbin |first5=T. |last6=Wycoff |first6=G. |last7=Bastian |first7=U. |last8=Schwekendiek |first8=P. |last9=Wicenec |first9=A. |display-authors=6 |date=March 2000 |title=The Tycho-2 catalogue of the 2.5&nbsp;million brightest stars |journal=Astronomy & Astrophysics |volume=355 |pages=L27–L30 |bibcode=2000A&A...355L..27H |issn=0004-6361 |s2cid=17128864}}</ref>
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[M33 X-7]] B (in [[Triangulum Galaxy]])
|70
|2,700,000
|18.7
|35,000
|Binary
|{{SIMBAD link|M33+X-7|SIMBAD}}
|<ref>{{Cite journal|last1=Orosz|first1=Jerome A.|last2=McClintock|first2=Jeffrey E.|last3=Narayan|first3=Ramesh|last4=Bailyn|first4=Charles D.|last5=Hartman|first5=Joel D.|last6=Macri|first6=Lucas|last7=Liu|first7=Jiefeng|last8=Pietsch|first8=Wolfgang|last9=Remillard|first9=Ronald A.|last10=Shporer|first10=Avi|last11=Mazeh|first11=Tsevi |display-authors=6 |date=October 2007|title=A 15.65-solar-mass black hole in an eclipsing binary in the nearby spiral galaxy M 33|journal=Nature|language=en|volume=449|issue=7164|pages=872–875|arxiv=0710.3165|bibcode=2007Natur.449..872O|doi=10.1038/nature06218|issn=0028-0836|pmid=17943124|s2cid=4311574}}</ref><ref>{{Cite journal|last1=Grimm|first1=H.-J.|last2=McDowell|first2=J.|last3=Zezas|first3=A.|last4=Kim|first4=D.-W.|last5=Fabbiano|first5=G.|date=December 2005|title=The X-Ray Binary Population in M33. I. Source List and Luminosity Function|journal=The Astrophysical Journal Supplement Series|language=en|volume=161|issue=2|pages=271–303|arxiv=astro-ph/0506353|bibcode=2005ApJS..161..271G|doi=10.1086/468185|issn=0067-0049|s2cid=119381693}}</ref>
|- style="text-align:center;"
| style="background: {{항성-색깔|WC}};text-align:left;" | [[Sk -69° 194]] A (in [[NGC 2033]] of [[Large Magellanic Cloud|LMC]])
|70
|160,000
|12.131<br/>{{small|(연성계 전체)}}
|45,000
|Evolution
|{{SIMBAD link|Sk+-69+194|SIMBAD}}
|<ref name=Massey2000/><ref name="Ulaczyk">{{Cite journal|last1=Ulaczyk |first1=K. |last2=Szymański |first2=M.K. |last3=Udalski |first3=A. |last4=Kubiak |first4=M. |last5=Pietrzyński |first5=G. |last6=Soszyński |first6=I. |last7=Wyrzykowski |first7=Ł. |last8=Poleski |first8=R. |last9=Gieren |first9=W. |last10=Walker |first10=A.R. |last11=Garcia-Varela |first11=A. |display-authors=6 |date=1 June 2013|title=Variable Stars from the OGLE-III Shallow Survey in the Large Magellanic Cloud|journal=Acta Astronomica|volume=63|issue=2|pages=159–179|arxiv=1306.4802|bibcode=2013AcA....63..159U|issn=0001-5237|s2cid=119228254}}</ref><ref name="Binary" group="lower-alpha" />
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[VFTS 125]] (in [[타란툴라 성운]] of [[Large Magellanic Cloud|LMC]])
|69.6
|164,000
|16.6
|55,200
|Spectroscopy
|{{SIMBAD link|VFTS+125|SIMBAD}}
|<ref name="schneider2018" /><ref name="Schild" />
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[HD 46150]] (in [[NGC 2244]] of [[Rosette Nebula]])
|69
|5,200
|6.73
|44,000
|Spectroscopy
|{{SIMBAD link|HD+46150|SIMBAD}}
|<ref name="fulltext" /><ref name="ducati" />
|- style="text-align:center;"
| style="background: {{항성-색깔|B}};text-align:left;" | [[Berkeley 87|HD 229059]] (in [[Berkeley 87]])
|69
|3,000
|8.7
|26,300
|Evolution
|{{SIMBAD link|HD+229059|SIMBAD}}
|<ref name=Massey2001/><ref name="ducati" />
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[ST2-3]] (in [[NGC 2044]] of [[Large Magellanic Cloud|LMC]])
|69
|160,000
|14.264
|44,900
|Evolution
|{{SIMBAD link|ST92+2-3|SIMBAD}}
|<ref name=Massey2000/><ref name=Bonanos/>
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[ST2-32]] (in [[NGC 2044]] of [[Large Magellanic Cloud|LMC]])
|69
|160,000
|13.903
|45,400
|Evolution
|{{SIMBAD link|ST92+2-32|SIMBAD}}
|<ref name=Massey2000/><ref name=Bonanos/>
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[W28-23]] (in [[NGC 2033]] of [[Large Magellanic Cloud|LMC]])
|69
|160,000
|13.702
|51,300
|Evolution
|{{SIMBAD link|W61+28-23|SIMBAD}}
|<ref name=Massey2000/><ref name="Zaritsky" />
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[HD 93403]] A (in [[트럼플러 16]] of [[용골자리 성운]])
|68.5
|10,400
|8.27<br/>{{small|(연성계 전체)}}
|39,300
|Binary
|{{SIMBAD link|HD+93403|SIMBAD}}
|<ref name="rauw2000">{{Cite journal |last1=Rauw |first1=G. |last2=Sana |first2=H. |last3=Gosset |first3=E. |last4=Vreux |first4=J.-M. |last5=Jehin |first5=E. |last6=Parmentier |first6=G. |date=August 2000|title=A new orbital solution for the massive binary system HD&nbsp;93403 |journal=Astronomy & Astrophysics|volume=360 |pages=1003–1010 |bibcode=2000A&A...360.1003R |issn=0004-6361 |s2cid=13886945}}</ref><ref name="zacharias" />
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[콜린더 228|HD 93130]] (in [[콜린더 228]] of [[용골자리 성운]])
|68
|10,000
|8.04
|39,900
|Evolution
|{{SIMBAD link|HD+93130|SIMBAD}}
|<ref name=Massey2001/><ref name="ducati" />
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[HM 1]]-8 (in [[HM 1]])
|68
|11,000
|12.52
|46,100
|Evolution
|{{SIMBAD link|Cl+HM+1+8|SIMBAD}}
|<ref name=Massey2001/><ref name=Reed/>
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[HSH95-47]] (in [[타란툴라 성운]] of [[Large Magellanic Cloud|LMC]])
|68
|163,000
|14.72
|43,500
|Evolution
|{{SIMBAD link|HSH95+47|SIMBAD}}
|<ref name="Brands2022" /><ref name="Doran2013" />
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[HSH95-48]] (in [[타란툴라 성운]] of [[Large Magellanic Cloud|LMC]])
|68
|163,000
|14.75
|46,500
|Evolution
|{{SIMBAD link|HSH95+48|SIMBAD}}
|<ref name=Brands2022/><ref name=crowther2016/>
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[웨스터하우트 51]]-61 (in [[웨스터하우트 51]])
|68
|20,000
|18.16<br/>{{small|(J&nbsp;대역)}}
|38,000
|Evolution
|{{SIMBAD link|SSTOERC+G049.4836-00.4060|SIMBAD}}
|<ref name=Bik/><ref name=2MASS/>
|- style="text-align:center;"
| style="background: {{항성-색깔|WC}};text-align:left;" | [[BAT99-93]] (in [[타란툴라 성운]] of [[Large Magellanic Cloud|LMC]])
|67
|165,000
|13.446
|45,000
|Spectroscopy
|{{SIMBAD link|BAT99+93|SIMBAD}}
|<ref name="hainich" /><ref name=Bonanos/>
|- style="text-align:center;"
| style="background: {{항성-색깔|B}};text-align:left;" | [[Sk -69° 200]] (in [[NGC 2033]] of [[Large Magellanic Cloud|LMC]])
|67
|160,000
|11.18
|26,300
|Evolution
|{{SIMBAD link|Sk+-69+200|SIMBAD}}
|<ref name=Massey2000/><ref name=Bonanos/>
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[아치스 성단|아치스]]-F18 (in [[아치스 성단]])
|66.9
|25,000
|16.7<br/>{{small|(J&nbsp;대역)}}
|36,900
|Spectroscopy
|{{SIMBAD link|FNG2002+18|SIMBAD}}
|<ref name=grafener/><ref name=Figer/>
|- style="text-align:center;"
| style="background: {{항성-색깔|WC}};text-align:left;" | [[아치스 성단|아치스]]-F4 (WR 102al in [[아치스 성단]])
|66.4
|25,000
|15.63<br/>{{small|(J&nbsp;대역)}}
|36,800
|Spectroscopy
|{{SIMBAD link|FNG2002+4|SIMBAD}}
|<ref name=grafener/><ref name=Figer/>
|- style="text-align:center;"
| style="background: {{항성-색깔|WC}};text-align:left;" | [[BAT99-59]] A (in [[NGC 2020]] of [[Large Magellanic Cloud|LMC]])
|66
|165,000
|13.186<br/>{{small|(연성계 전체)}}
|71,000
|Spectroscopy
|{{SIMBAD link|BAT99+59|SIMBAD}}
|<ref name=hainich/><ref name=Bonanos/><ref name="Binary" group="lower-alpha" />
|- style="text-align:center;"
| style="background: {{항성-색깔|WC}};text-align:left;" | [[BAT99-104]] (in [[타란툴라 성운]] of [[Large Magellanic Cloud|LMC]])
|66
|165,000
|12.5
|63,000
|Spectroscopy
|{{SIMBAD link|BAT99+104|SIMBAD}}
|<ref name=hainich/><ref name=Bonanos/>
|- style="text-align:center;"
| style="background: {{항성-색깔|WC}};text-align:left;" | [[HD 5980]] B (in [[NGC 346]] of [[Small Magellanic Cloud|SMC]])
|66
|200,000
|11.31<br/>{{small|(연성계 전체)}}
|45,000
|Trinary
|{{SIMBAD link|HD+5980|SIMBAD}}
|<ref name="shenar">{{cite journal |last1=Shenar |first1=T. |last2=Hainich |first2=R. |last3=Todt |first3=H. |last4=Sander |first4=A. |last5=Hamann |first5=W.-R. |last6=Moffat |first6=A.F.J. |last7=Eldridge |first7=J.J. |last8=Pablo |first8=H.|last9=Oskinova |first9=L.M. |last10=Richardson |first10=N.D. |display-authors=6 |date=July 2016|title=Wolf-Rayet stars in the Small Magellanic Cloud: II. Analysis of the binaries |journal=Astronomy & Astrophysics |volume=591 |page=A22 |arxiv=1604.01022 |bibcode=2016A&A...591A..22S |doi=10.1051/0004-6361/201527916 |issn=0004-6361 |s2cid=119255408}}</ref><ref name="tycho2" />
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[HD 190429]] A (near [[Barnard 146]])
|66
|66
|7,800
|-
|6.63<br/>{{small|(연성계 전체)}}
|bgcolor="#aabfff"|[[LBV 1806-20]] A + B
|46,000
|A=65, B=65
|Binary
|-
|{{SIMBAD link|HD+190429A|SIMBAD}}
|bgcolor="#aabfff"|[[아치스 성단|아치스]]-F28
|<ref name="bouret2">{{cite journal |last1=Bouret |first1=J.-C. |last2=Hillier |first2=D.J. |last3=Lanz |first3=T. |last4=Fullerton |first4=A.W. |year=2012 |title=Properties of galactic early-type O-supergiants: A combined FUV-UV and optical analysis |journal=[[Astronomy & Astrophysics]] |volume=544 |page=A67 |arxiv=1205.3075 |bibcode=2012A&A...544A..67B |doi=10.1051/0004-6361/201118594 |s2cid=119280104}}</ref><ref name="ducati" />
|66–76
|- style="text-align:center;"
|-
| style="background: {{항성-색깔|O}};text-align:left;" | [[LH 31]]-1003 (in [[NGC 1858]] of [[Large Magellanic Cloud|LMC]])
|bgcolor="#aabfff"|[[LH54-425]] A + B
|66
|A=62, B=37
|160,000
|-
|13.186
|bgcolor="#aabfff"|[[아치스 성단|아치스]]-F21
|41,900
|56–70
|Evolution
|-
|{{SIMBAD link|L72+LH+31-1003|SIMBAD}}
|bgcolor="#aabfff"|[[아치스 성단|아치스]]-F10
|<ref name=Massey2000/><ref name=Bonanos/>
|55–69
|- style="text-align:center;"
|-
| style="background: {{항성-색깔|O}};text-align:left;" | [[LH 114]]-7 (in [[N70 (nebula)|N70]] of [[Large Magellanic Cloud|LMC]])
|bgcolor="#aabfff"|[[HD 148937]]<ref name=wade>{{저널 인용
|66
| doi = 10.1111/j.1365-2966.2011.19897.x
|160,000
| title = The spectral variability and magnetic field characteristics of the Of?p star HD 148937★
|13.66
| journal = Monthly Notices of the Royal Astronomical Society
|50,000
| volume = 419
|Spectroscopy
| issue = 3
|{{SIMBAD link|L72+LH+114-7|SIMBAD}}
| pages = 2459
|<ref name=fulltext/><ref name=Bonanos/><ref group="lower-alpha">N70 is an emission nebula in Large Magellanic Cloud.</ref>
| year = 2012
|- style="text-align:center;"
| last1 = Wade | first1 = G. A.
| style="background: {{항성-색깔|O}};text-align:left;" | [[피스미스 24-1]]SW (in [[피스미스 24]] of [[NGC 6357]])
| last2 = Grunhut | first2 = J.
|66
| last3 = Gräfener | first3 = G.
|6,500
| last4 = Howarth | first4 = I. D.
|11.1
| last5 = Martins | first5 = F.
|40,000
| last6 = Petit | first6 = V.
|Binary
| last7 = Vink | first7 = J. S.
|{{SIMBAD link|CL+PISMIS+24-1SW|SIMBAD}}
| last8 = Bagnulo | first8 = S.
|<ref name=fang/><ref name=skiff/>
| last9 = Folsom | first9 = C. P.
|- style="text-align:center;"
| last10 = Nazé | first10 = Y.
| style="background: {{항성-색깔|WC}};text-align:left;" | [[BAT99-126]] (in [[NGC 2081]] of [[Large Magellanic Cloud|LMC]])
| last11 = Walborn | first11 = N. R.
|65
| last12 = Townsend | first12 = R. H. D.
|165,000
| last13 = Evans | first13 = C. J.
|13.166
}}</ref>
|71,000
|Spectroscopy
|{{SIMBAD link|BAT99+126|SIMBAD}}
|<ref name=hainich/><ref name=Bonanos/>
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[HSH95-40]] (in [[Tarantula Nebula]] of [[Large Magellanic Cloud|LMC]])
|65
|163,000
|14.56
|47,500
|Evolution
|{{SIMBAD link|HSH95+40|SIMBAD}}
|<ref name="Brands2022" /><ref name="Doran2013" />
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[HSH95-58]] (in [[Tarantula Nebula]] of [[Large Magellanic Cloud|LMC]])
|65
|163,000
|14.8
|47,500
|Evolution
|{{SIMBAD link|HSH95+58|SIMBAD}}
|<ref name="Brands2022" /><ref name="Doran2013" />
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[HSH95-89]] (in [[Tarantula Nebula]] of [[Large Magellanic Cloud|LMC]])
|65
|163,000
|14.76
|44,000
|Spectroscopy
|{{SIMBAD link|HSH95+89|SIMBAD}}
|<ref name="crowther2016" />
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[VFTS 63]] (in [[Tarantula Nebula]] of [[Large Magellanic Cloud|LMC]])
|65
|164,000
|14.4
|42,200
|Spectroscopy
|{{SIMBAD link|VFTS+63|SIMBAD}}
|<ref name="best" /><ref name="Schild" />
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[VFTS 145]] (in [[Tarantula Nebula]] of [[Large Magellanic Cloud|LMC]])
|65
|164,000
|14.3
|39,800
|Spectroscopy
|{{SIMBAD link|VFTS+145|SIMBAD}}
|<ref name="best" /><ref name="Doran2013" />
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[VFTS 518]] (in [[Tarantula Nebula]] of [[Large Magellanic Cloud|LMC]])
|65
|164,000
|15.11
|44,700
|Spectroscopy
|{{SIMBAD link|VFTS+518|SIMBAD}}
|<ref name=best/><ref name=Doran2013/>
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[웨스터하우트 49]]-8 (in [[웨스터하우트 49]])
|65
|36,200
|15.617<br/>{{small|(J&nbsp;대역)}}
|40,700
|Evolution
|{{SIMBAD link|WBB2016+8|SIMBAD}}
|<ref name=Wu2016/><ref name=2MASS/>
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[BD+43° 3654]] ([[폭주성]] from [[백조자리 OB2]])
|64.6
|5,400
|10.06
|40,400
|Evolution
|{{SIMBAD link|BD%2B43+3654|SIMBAD}}
|<ref name="comeron">{{Cite journal|last1=Comerón|first1=F.|last2=Pasquali|first2=A.|date=July 2012|title=New members of the massive stellar population in Cygnus|journal=Astronomy & Astrophysics|volume=543|page=A101|bibcode=2012A&A...543A.101C|doi=10.1051/0004-6361/201219022|issn=0004-6361|s2cid=73520813|doi-access=free}}</ref><ref name="tycho2" />
|- style="text-align:center;"
| style="background: {{항성-색깔|WC}};text-align:left;" | [[BAT99-129]] A (in [[DEM L294]] of [[Large Magellanic Cloud|LMC]])
|64
|165,000
|14.701<br/>{{small|(연성계 전체)}}
|79,000
|Spectroscopy
|{{SIMBAD link|BAT99+129|SIMBAD}}
|<ref name="hainich" /><ref name=Bonanos/><ref group="lower-alpha">DEM L294 is a H II region in Large Magellanic Cloud.</ref><ref name="Binary" group="lower-alpha" />
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[HSH95-50]] (in [[Tarantula Nebula]] of [[Large Magellanic Cloud|LMC]])
|64
|163,000
|14.65
|47,000
|Evolution
|{{SIMBAD link|HSH95+50|SIMBAD}}
|<ref name=Brands2022/><ref name=Doran2013/>
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[Sk -69° 25]] (in [[NGC 1748]] of [[Large Magellanic Cloud|LMC]])
|64
|160,000
|11.886
|43,600
|Evolution
|{{SIMBAD link|Sk+-69+25|SIMBAD}}
|<ref name=Massey2000/><ref name=Bonanos/>
|- style="text-align:center;"
| style="background: {{항성-색깔|B}};text-align:left;" | [[트럼플러 27]]-23 (in [[트럼플러 27]])
|64
|3,900
|10.09
|27,500
|Evolution
|{{SIMBAD link|Cl+Trumpler+27+23|SIMBAD}}
|<ref name=Massey2001/><ref name=zacharias/>
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[웨스터하우트 49]]-5 (in [[웨스터하우트 49]])
|64
|36,200
|15.623<br/>{{small|(J&nbsp;대역)}}
|42,700
|Evolution
|{{SIMBAD link|WBB2016+5|SIMBAD}}
|<ref name=Wu2016/><ref name=2MASS/>
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[HD 46223]] (in [[NGC 2244]] of [[Rosette Nebula]])
|63
|5,200
|7.28
|46,000
|Spectroscopy
|{{SIMBAD link|HD+46223|SIMBAD}}
|<ref name="fulltext" /><ref name="ducati" />
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[HD 64568]] (in [[NGC 2467]] of [[Puppis OB2]])
|63
|16,000
|9.39
|54,000
|Spectroscopy
|{{SIMBAD link|HD+64568|SIMBAD}}
|<ref name="fulltext" /><ref name="zacharias" />
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[트럼플러 16|HD 303308]] (in [[트럼플러 16]] of [[용골자리 성운]])
|63
|9,200
|8.17
|51,300
|Evolution
|{{SIMBAD link|HD+303308|SIMBAD}}
|<ref name=Massey2001/><ref name="zacharias" />
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[HR 6187]] A (in [[NGC 6193]] of [[Ara OB1]])
|63
|4,300
| style="background:lightblue;color:darkblue;" |'''5.54'''<br/>{{small|(연성계 전체)}}
|46,500
|Septenary
|{{SIMBAD link|HR+6187|SIMBAD}}
|<ref name="krticka">{{Cite journal |last1=Krtička |first1=J. |last2=Kubát |first2=J. |last3=Krtičková |first3=I. |date=July 2015 |title=X-ray irradiation of the winds in binaries with massive components |journal=Astronomy & Astrophysics |volume=579 |page=A111 |arxiv=1505.03411 |bibcode=2015A&A...579A.111K |doi=10.1051/0004-6361/201525637 |issn=0004-6361 |s2cid=119120927}}</ref><ref name="ducati" />
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[LH 10]]-3058 (in [[NGC 1763]] of [[Large Magellanic Cloud|LMC]])
|63
|160,000
|14.089
|54,000
|Spectroscopy
|{{SIMBAD link|PGMW+3058|SIMBAD}}
|<ref name="fulltext" /><ref name=Bonanos/>
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[ST5-71]] (in [[NGC 2074]] of [[Large Magellanic Cloud|LMC]])
|63
|160,000
|13.266
|45,400
|Evolution
|{{SIMBAD link|ST92+5-71|SIMBAD}}
|<ref name=Massey2000/><ref name=Bonanos/>
|- style="text-align:center;"
| style="background: {{항성-색깔|WC}};text-align:left;" | [[AB9 (항성)|AB9]] (in [[DEM S80]] of [[Small Magellanic Cloud|SMC]])
|62
|197,000
|15.431
|100,000
|Spectroscopy
|{{SIMBAD link|SMC+AB+9|SIMBAD}}
|<ref name=Hainich2015/><ref name="spitzer" /><ref group="lower-alpha">DEM S80 is a H II region in Small Magellanic Cloud.</ref>
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[Brey 32]] B (in [[NGC 1966]] of [[Large Magellanic Cloud|LMC]])
|62
|165,000
|12.32<br/>{{small|(연성계 전체)}}
|43,600
|Evolution
|{{SIMBAD link|Brey+32|SIMBAD}}
|<ref name=Massey2000/><ref name="zacharias" />
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[트럼플러 14|HD 93160]] (in [[트럼플러 14]] of [[용골자리 성운]])
|62
|8,000
|7.6
|42,700
|Evolution
|{{SIMBAD link|HD+93160|SIMBAD}}
|<ref name=Massey2001/><ref name="ducati" />
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[HSH95-35]] (in [[Tarantula Nebula]] of [[Large Magellanic Cloud|LMC]])
|62
|163,000
|14.43
|47,500
|Evolution
|{{SIMBAD link|HSH95+35|SIMBAD}}
|<ref name=Brands2022/><ref name=Doran2013/>
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[LH 41]]-1017 (in [[NGC 1910]] of [[Large Magellanic Cloud|LMC]])
|62
|160,000
|12.266
|42,700
|Evolution
|{{SIMBAD link|L72+LH+41-1017|SIMBAD}}
|<ref name=Massey2000/><ref name=Bonanos/>
|- style="text-align:center;"
| style="background: {{항성-색깔|WC}};text-align:left;" | [[머서 30]]-6a A (WR 46-4 A in [[머서 30]] of [[Dragonfish Nebula]])
|62
|40,000
|10.39<br/>{{small|(J&nbsp;대역)}}
|29,900
|Evolution
|{{SIMBAD link|DNB2016+Mc30-6a|SIMBAD}}
|<ref name=Fuente/><ref group=lower-alpha name=Mc30/><ref name="Binary" group="lower-alpha" />
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[ST4-18]] (in [[NGC 2081]] of [[Large Magellanic Cloud|LMC]])
|62
|160,000
|13.639
|44,800
|Evolution
|{{SIMBAD link|ST92+4-18|SIMBAD}}
|<ref name=Massey2000/><ref name=Bonanos/>
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[VFTS 664]] (in [[Tarantula Nebula]] of [[Large Magellanic Cloud|LMC]])
|62
|164,000
|13.937
|39,900
|Spectroscopy
|{{SIMBAD link|VFTS+664|SIMBAD}}
|<ref name=best/><ref name=Bonanos/>
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[백조자리 OB9|HD 229196]] (in [[백조자리 OB9]])
|61.6
|5,000
|8.59
|40,900
|Evolution
|{{SIMBAD link|HD+229196|SIMBAD}}
|<ref name=comeron/><ref name=Reed/>
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[AB8 (항성)|AB8]] B (in [[NGC 602]] of [[Small Magellanic Cloud|SMC]])
|61
|197,000
|12.83<br/>{{small|(연성계 전체)}}
|45,000
|Binary
|{{SIMBAD link|SMC+AB+8|SIMBAD}}
|<ref name="shenar" /><ref>{{Cite journal|last=Massey|first=Philip|date=July 2002|title=A UBVR CCD Survey of the Magellanic Clouds|journal=The Astrophysical Journal Supplement Series|language=en|volume=141|issue=1|pages=81–122|arxiv=astro-ph/0110531|bibcode=2002ApJS..141...81M|doi=10.1086/338286|issn=0067-0049|s2cid=119447348}}</ref>
|- style="text-align:center;"
| style="background: {{항성-색깔|WC}};text-align:left;" | [[BAT99-79]] A (in [[NGC 2044]] of [[Large Magellanic Cloud|LMC]])
|61
|165,000
|13.486<br/>{{small|(연성계 전체)}}
|42,000
|Spectroscopy
|{{SIMBAD link|BAT99+79|SIMBAD}}
|<ref name="hainich" /><ref name=Bonanos/><ref name="Binary" group="lower-alpha" />
|- style="text-align:center;"
| style="background: {{항성-색깔|WC}};text-align:left;" | [[HD 5980]] A (in [[NGC 346]] of [[Small Magellanic Cloud|SMC]])
|61
|200,000
|11.31<br/>{{small|(연성계 전체)}}
|21,000–53,000
|Trinary
|{{SIMBAD link|HD+5980|SIMBAD}}
|<ref name=shenar/><ref name=tycho2/>
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[LH 41]]-18 (in [[NGC 1910]] of [[Large Magellanic Cloud|LMC]])
|61
|160,000
|12.586
|38,500
|Evolution
|{{SIMBAD link|L72+LH+41-18|SIMBAD}}
|<ref name=Massey2000/><ref name=Bonanos/>
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[머서 30]]-9 A (in [[머서 30]] of [[Dragonfish Nebula]])
|61
|40,000
|12.25<br/>{{small|(J&nbsp;대역)}}
|34,500
|Evolution
|{{SIMBAD link|DNB2016+Mc30-9|SIMBAD}}
|<ref name=Fuente/><ref group=lower-alpha name=Mc30/><ref name="Binary" group="lower-alpha" />
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[ST5-25]] (in [[NGC 2074]] of [[Large Magellanic Cloud|LMC]])
|61
|160,000
|13.551
|48,600
|Evolution
|{{SIMBAD link|ST92+5-25|SIMBAD}}
|<ref name=Massey2000/><ref name=Zaritsky/>
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[VFTS 422]] (in [[Tarantula Nebula]] of [[Large Magellanic Cloud|LMC]])
|61
|164,000
|15.14
|39,800
|Spectroscopy
|{{SIMBAD link|VFTS+422|SIMBAD}}
|<ref name=best/><ref name=Doran2013/>
|- style="text-align:center;"
| style="background: {{항성-색깔|WC}};text-align:left;" | [[다섯쌍둥이 성단|WR 102hb]] (in [[다섯쌍둥이 성단]])
|61
|26,000
|13.9<br/>{{small|(J&nbsp;대역)}}
|25,100
|Evolution
|{{SIMBAD link|WR+102hb|SIMBAD}}
|<ref name=Liermann>{{Cite journal |last1=Liermann |first1=Adriane|last2=Hamann |first2=Wolf-Rainer |last3=Oskinova |first3=Lidia M. |last4=Todt |first4=Helge |date=January 2011 |title=High-mass stars in the Galactic center Quintuplet cluster |journal=Société Royale des Sciences de Liège, Bulletin |volume=80 |pages=160–164 |bibcode=2011BSRSL..80..160L |issn=0037-9565 |s2cid=116895316}}</ref><ref name="qc">{{Cite journal|last1=Clark |first1=J.S. |last2=Lohr |first2=M.E. |last3=Patrick |first3=L.R. |last4=Najarro |first4=F. |last5=Dong |first5=H. |last6=Figer |first6=D.F. |date=October 2018 |title=An updated stellar census of the Quintuplet cluster |journal=Astronomy & Astrophysics |volume=618 |page=A2 |arxiv=1805.10139 |bibcode=2018A&A...618A...2C |doi=10.1051/0004-6361/201833041 |issn=0004-6361 |s2cid=53501337}}</ref>
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[Sk -67° 166]] (in [[GKK-A144]] of [[Large Magellanic Cloud|LMC]])
|60.68
|160,000
|12.22
|41,800
|Spectroscopy
|{{SIMBAD link|Sk+-67+166|SIMBAD}}
|<ref name=Massa2017/><ref name=Bonanos/><ref group="lower-alpha" name="A144">GKK-A144 is a stellar association in Large Magellanic Cloud.</ref>
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[Sk -67° 167]] (in [[GKK-A144]] of [[Large Magellanic Cloud|LMC]])
|60.68
|160,000
|12.586
|41,800
|Spectroscopy
|{{SIMBAD link|Sk+-67+167|SIMBAD}}
|<ref name=Massa2017/><ref name=Bonanos/><ref group=lower-alpha name=A144/>
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[Sk -71° 46]] (in [[BSDL 2242]] of [[Large Magellanic Cloud|LMC]])
|60.68
|160,000
|13.241
|41,800
|Spectroscopy
|{{SIMBAD link|Sk+-71+46|SIMBAD}}
|<ref name=Massa2017/><ref name=Bonanos/><ref group="lower-alpha">BSDL 2242 is a star cluster in Large Magellanic Cloud.</ref>
|- style="text-align:center;"
| style="background: {{항성-색깔|WC}};text-align:left;" | [[Brey 10]] (in [[NGC 1770]] of [[Large Magellanic Cloud|LMC]])
|60
|165,000
|12.69
|117,000
|Evolution
|{{SIMBAD link|Brey+10|SIMBAD}}
|<ref name=Massey2000/><ref name=zacharias/>
|- style="text-align:center;"
| style="background: {{항성-색깔|WC}};text-align:left;" | [[Brey 94]] A (in [[NGC 2081]] of [[Large Magellanic Cloud|LMC]])
|60
|165,000
|12.996<br/>{{small|(연성계 전체)}}
|83,000
|Evolution
|{{SIMBAD link|Brey+94|SIMBAD}}
|<ref name=Massey2000/><ref name=Bonanos/><ref name="Binary" group="lower-alpha" />
|- style="text-align:center;"
| style="background: {{항성-색깔|WC}};text-align:left;" | [[Brey 95a]] A (in [[NGC 2081]] of [[Large Magellanic Cloud|LMC]])
|60
|165,000
|12.2<br/>{{small|(연성계 전체)}}
|83,000
|Evolution
|{{SIMBAD link|Brey+95a|SIMBAD}}
|<ref name=Massey2000/><ref name=Testor>{{Cite journal |last1=Testor |first1=G. |last2=Niemela |first2=V. |date=June 1998 |title=The OB associations LH 101 and LH 104 in the HII region N158 of the LMC |journal=Astronomy and Astrophysics Supplement Series |volume=130 |issue=3 |pages=527–538 |bibcode=1998A&AS..130..527T |doi=10.1051/aas:1998241 |issn=0365-0138 |s2cid=55801387 |doi-access=free}}</ref><ref name="Binary" group="lower-alpha" />
|- style="text-align:center;"
| style="background: {{항성-색깔|O}};text-align:left;" | [[HSH95-55]] (in [[Tarantula Nebula]] of [[Large Magellanic Cloud|LMC]])
|60
|163,000
|14.74
|47,500
|Evolution
|{{SIMBAD link|HSH95+55|SIMBAD}}
|<ref name=Brands2022/><ref name=Doran2013/>
|- style="text-align:center;"
| style="background: {{항성-색깔|WC}};text-align:left;" | [[머서 30]]-7 A (WR 46-5 A in [[머서 30]] of [[Dragonfish Nebula]])
|60
|40,000
|11.516<br/>{{small|(J&nbsp;대역)}}
|41,400
|Evolution
|{{SIMBAD link|DNB2016+Mc30-7|SIMBAD}}
|<ref name=Fuente/><ref group=lower-alpha name=Mc30/><ref name="Binary" group="lower-alpha" />
|- style="text-align:center;"
| style="background: {{항성-색깔|WC}};text-align:left;" | [[R134 (항성)|R134]] (in [[Tarantula Nebula]] of [[Large Magellanic Cloud|LMC]])
|60
|164,000
|12.75
|39,800
|Spectroscopy
|{{SIMBAD link|RMC134|SIMBAD}}
|<ref name=best/><ref name=Doran2013/>
|- style="text-align:center;"
| style="background: {{항성-색깔|B}};text-align:left;" | [[R142 (항성)|R142]] (in [[Tarantula Nebula]] of [[Large Magellanic Cloud|LMC]])
|60
|164,000
|11.82
|18,000
|Spectroscopy
|{{SIMBAD link|RMC142|SIMBAD}}
|<ref name=McEvoy/><ref name=Doran2013/>
|- style="text-align:center;"
| style="background: {{항성-색깔|WN}};text-align:left;" | [[R143 (항성)|R143]] (in [[Tarantula Nebula]] of [[Large Magellanic Cloud|LMC]])
|60
|160,000
|12.014
|18,000–36,000
|Evolution
|{{SIMBAD link|RMC143|SIMBAD}}
|<ref name=Smith2015/><ref name=Bonanos/>
|- style="text-align:center;"
| style="background: {{항성-색깔|WN}};text-align:left;" | [[Sk -69° 142a]] (in [[NGC 1983]] of [[Large Magellanic Cloud|LMC]])
|60
|160,000
|11.093
|34,000
|Evolution
|{{SIMBAD link|Sk+-69+142a|SIMBAD}}
|<ref name=Smith2015/><ref name=Ulaczyk/>
|- style="text-align:center;"
| style="background: {{항성-색깔|B}};text-align:left;" | [[Sk -69° 259]] (in [[NGC 2081]] of [[Large Magellanic Cloud|LMC]])
|60
|160,000
|11.93
|23,000
|Evolution
|{{SIMBAD link|Sk+-69+259|SIMBAD}}
|<ref name=Massey2000/><ref name=zacharias/>
|- style="text-align:center;"
| style="background: {{항성-색깔|WN}};text-align:left;" | [[Var 83]] (in [[Triangulum Galaxy]])
|60
|3,000,000
|16.027
|18,000–37,000
|Evolution
|{{SIMBAD link|VHK+83|SIMBAD}}
|<ref name=burggraf>{{cite conference |last1=Burggraf |first1=B. |last2=Weis |first2=K. |last3=Bomans |first3=D.J. |date=December 2006 |title=LBVs in M33: Their environments and ages |book-title=Stellar Evolution at Low Metallicity: Mass loss, explosions, cosmology |series=ASP Conference Series |volume=353 |page=245 |bibcode=2006ASPC..353..245B |issn=1050-3390 |s2cid=230292777 |publisher=[[Astronomical Society of the Pacific]]}}</ref><ref>{{cite journal |last1=Massey |first1=Philip |last2=Neugent |first2=Kathryn F. |last3=Smart |first3=Brianna M. |date=19 August 2016 |title=A spectroscopic survey of massive stars in M31 and M33 |journal=[[The Astronomical Journal]] |volume=152 |issue=3 |page=62 |arxiv=1604.00112 |bibcode=2016AJ....152...62M |doi=10.3847/0004-6256/152/3/62 |issn=1538-3881 |s2cid=35672588 |doi-access=free }}</ref>
|- style="text-align:center;"
| style="background: {{항성-색깔|B}};text-align:left;" | [[VFTS 430]] (in [[Tarantula Nebula]] of [[Large Magellanic Cloud|LMC]])
|60
|60
|164,000
|15.11
|24,500
|Spectroscopy
|{{SIMBAD link|VFTS+430|SIMBAD}}
|<ref name=McEvoy/><ref name=Doran2013/>
|-
|-
|bgcolor="#9bb0ff"|[[아치스 성단|아치스]]-F14
|bgcolor="#9bb0ff"|[[아치스 성단|아치스]]-F14

2024년 1월 18일 (목) 01:11 판

무거운 별 주위를 물질이 둘러싸 빛을 가리고 있다. 천체 예술가의 상상화
용골자리 에타의 질량은 태양의 약 150배로, 이는 항성이 지닐 수 있는 질량의 상한선에 가깝다.

아래 표는 지금까지 관측된 별들 중 질량이 큰 것들을 순서대로 정렬한 것이다. 단위는 태양질량이다.

질량은 항성의 모든 것을 결정하는 가장 중요한 요소이다. 질량은 항성의 화학적 조성 상태와 맞물려 그 별의 밝기, 물리적 크기, 운명까지 결정한다. 질량이 큰 별의 경우 대부분 초신성 폭발로 일생을 마치며, 블랙홀을 형성하기도 한다.

불확실한 점 및 논쟁거리

아래 표에 수록된 항성들의 질량은 이론 및 표면 온도와 절대 광도를 이용하여 복잡한 계산을 수행하여 얻은 값이다. 따라서 수록된 질량들은 확실한 수치가 아니다(이론 및 측정자료들이 구할 수 있는 한계점에서 나온 것이다). 이론과 측정값 모두 틀릴 수 있다. 대표적 예로 세페우스자리 VV A가 있는데, 이 별의 물리적 수치를 어떤 모형을 통해 구하느냐에 따라 질량은 태양의 25 ~ 40배 또는 100배까지 판이하게 달라진다.

그 중에서 가장 신빙성 있는 질량값은 A1과 WR20a+b로 직접 측정하여 얻은 것이다. 둘 다 쌍성계의 일원으로, 쌍성계 구성원들의 공전 움직임을 분석하여, 케플러의 행성 운동법칙에 의거하여 각각의 질량을 구할 수 있었다. 이들의 질량을 알아내는 데 광도곡선 및 시선 속도도 이용되었는데, 이는 둘 다 식쌍성이었기 때문이다.

질량이 큰 별은 드물다. 아래 수록된 모든 별들은 태양계에서 수천 광년 이상 떨어져 있으며 보통 홀로 존재하기 때문에 질량 측정을 힘들게 만든다. 멀리 떨어져 있다는 것 외에도 무거운 별들 주변에는 자신이 방출한 가스로 인해 성운이 형성되어 있기 때문에 항성의 빛을 가려 정확한 표면 온도와 밝기, 내부 화학 조성에 대한 자료를 구하기 힘들게 만든다. 따라서 아래 목록의 자료값들은 대부분 논란 중에 있으며 연구 결과에 따라 수치는 재조정된다.

목록

범례
볼프-레이에별
밝은 청색변광성
O형 항성
B형 항성

다음 두 목록은 산개성단, OB 성협, H II 영역의 별을 포함하여 알려진 별 중 몇 가지를 수록한다. 목록의 상당수의 별들은 높은 광도에도 불구하고 맨눈으로 관찰하기에는 너무 멀리 떨어져 있으며 적어도 맨눈으로 가끔 볼 수 있는 별은 겉보기 등급(6.5 이상)이 파란색으로 강조되어 있다.

첫 번째 목록은 60 M☉ 이상으로 추정되는 별으로 그 중 대부분이 수록되며 두 번째 목록에는 비교를 위해 60 M☉ 미만의 주목할만한 별이 수록되어 있다. 데이터의 불확실성에 대한 정보를 제공하기 위해 각 별의 질량을 결정하는 데 사용되는 방법이 포함되어있으며 쌍성의 질량은 훨씬 더 정확하게 결정될 수 있다. 아래 나열된 질량은 별의 초기 질량이 아닌 현재 질량이다.

이 목록은 아직 미완성입니다. 여러분이 편집하여 채워 주세요.
60 M☉ 이상의 항성들
항성 이름 질량

(M☉, 태양 = 1)

대략 태양계로부터의 거리(광년) 겉보기등급 유효온도 (K) 분석 방식 링크 참고문헌
BAT99-98 (in 타란툴라 성운 of LMC) 226 165,000 13.37 45,000 Spectroscopy SIMBAD [1][2]
R136a1 (in 타란툴라 성운 of LMC) 196 163,000 12.23 46,000 Evolution SIMBAD [3][4]
멜닉 42 (in 타란툴라 성운 of LMC) 189 163,000 12.78 47,300 Spectroscopy SIMBAD [5][2]
VFTS 1022 (in 타란툴라 성운 of LMC) 178 164,000 13.47 42,200 Spectroscopy SIMBAD [5][2]
웨스터하우트 51-57 (in 웨스터하우트 51) 160 20,000 16.66
(J 대역) 		42,700 Evolution [6]
R136a3 (in 타란툴라 성운 of LMC) 155 163,000 12.97 50,000 Evolution SIMBAD [3][4]
VFTS 682 (in 타란툴라 성운 of LMC) 153 164,000 16.08 52,200 Spectroscopy SIMBAD [7][2]
HD 15558 A (in IC 1805 of Heart Nebula) 152 24,400 7.87
(연성계 전체) 		39,500 Binary SIMBAD [8][9]
R136a2 (in 타란툴라 성운 of LMC) 151 163,000 12.34 50,000 Evolution SIMBAD [3][4]
웨스터하우트 51-3 (in 웨스터하우트 51) 148 20,000 17.79
(J 대역) 		39,800 Evolution SIMBAD [6]
멜닉 34 A (in 타란툴라 성운 of LMC) 147 163,000 13.09
(연성계 전체) 		53,000 Binary SIMBAD [10][2]
VFTS 482 (in 타란툴라 성운 of LMC) 145 164,000 12.95 42,200 Spectroscopy SIMBAD [5][2]
R136c (in 타란툴라 성운 of LMC) 142 163,000 13.43 51,000 Evolution SIMBAD [11][2]
VFTS 1021 (in 타란툴라 성운 of LMC) 141 164,000 13.35 39,800 Spectroscopy SIMBAD [5][2]
LH 10-3209 A (in NGC 1763 of LMC) 140 160,000 11.859
(연성계 전체) 		42,500 Spectroscopy SIMBAD [12][13][a]
VFTS 506 (in 타란툴라 성운 of LMC) 138 164,000 13.31 47,300 Spectroscopy SIMBAD [7][2]
멜닉 34 B (in 타란툴라 성운 of LMC) 136 163,000 13.09
(연성계 전체) 		53,000 Binary SIMBAD [10][2]
웨스터하우트 51d (in 웨스터하우트 51) 135 20,000 15.11
(J 대역) 		42,700 Evolution [6]
VFTS 545 (in Tarantula Nebula of LMC) 133 164,000 13.32 47,300 Spectroscopy SIMBAD [5][2]
HD 97950 B (WR 43b in HD 97950 of NGC 3603) 132 24,800 11.33 42,000 Spectroscopy SIMBAD [14][15]
HD 269810 (in NGC 2029 of LMC) 130 163,000 12.22 52,500 Spectroscopy SIMBAD [16][17]
R136a7 (in Tarantula Nebula of LMC) 127 163,000 13.97 54,000 Evolution SIMBAD [18][2]
WR 42e (in HD 97950 of NGC 3603) 123 25,000 14.53 43,000 Ejection SIMBAD [19][b]
HD 97950 A1a (WR 43a A in HD 97950 of NGC 3603) 120 24,800 11.18
(연성계 전체) 		42,000 Binary SIMBAD [14][15]
LSS 4067 (in HM 1) 120 11,000 11.44 40,000 Evolution SIMBAD [20][21]
WR 93 (in 피스미스 24 of NGC 6357) 120 5,900 10.68 71,000 Evolution SIMBAD [20][9]
Sk -69° 212 (in NGC 2044 of LMC) 119 160,000 12.416 45,400 Evolution SIMBAD [22][13]
Sk -69° 249 A (in NGC 2074 of LMC) 119 160,000 12.02
(연성계 전체) 		38,900 Evolution SIMBAD [22][23]
ST5-31 (in NGC 2074 of LMC) 119 160,000 12.273 50,700 Evolution SIMBAD [22][24]
R136a5 (in Tarantula Nebula of LMC) 116 157,000 13.71 48,000 Evolution SIMBAD [18][2]
MSP 183 (in 웨스터룬드 2) 115 20,000 13.878 46,300 Spectroscopy SIMBAD [25][26]
WR 24 (in 콜린더 228 of 용골자리 성운) 114 14,000 6.48 50,100 Evolution SIMBAD [27][28]
HD 97950 C1 (WR 43c A in HD 97950 of NGC 3603) 113 24,800 11.89
(연성계 전체) 		44,000 Spectroscopy SIMBAD [14][15][a]
아치스-F9 (WR 102ae in 아치스 성단) 111.3 25,000 16.1
(J 대역) 		36,600 Spectroscopy SIMBAD [29][30]
백조자리 OB2 #12 A (in 백조자리 OB2) 110 5,200 11.702
(연성계 전체) 		13,700 Spectroscopy SIMBAD [31][32][a]
HD 93129 Aa (in 트럼플러 14 of 용골자리 성운) 110 7,500 6.9
(연성계 전체) 		42,500 Trinary SIMBAD [33][9]
HSH95-36 (in Tarantula Nebula of LMC) 110 163,000 14.41 49,500 Evolution SIMBAD [18][2]
R146 (in Tarantula Nebula of LMC) 109 164,000 13.11 63,000 Spectroscopy SIMBAD [1][2]
R136a4 (in Tarantula Nebula of LMC) 108 157,000 13.41 50,000 Evolution SIMBAD [18][2]
VFTS 621 (in Tarantula Nebula of LMC) 107 164,000 15.39 54,000 Spectroscopy SIMBAD [5][2]
R136a6 (in Tarantula Nebula of LMC) 105 157,000 13.35 52,000 Evolution SIMBAD [18][2]
웨스터하우트 49-3 (in 웨스터하우트 49) 105 36,200 16.689
(J 대역) 		40,700 Evolution SIMBAD [34][35]
WR 21a A (폭주성 from 웨스터룬드 2) 103.6 26,100 12.661 (연성계 전체) 45,000 Binary SIMBAD [36][17]
R99 (in N44 of LMC) 103 164,000 11.52 28,000 Spectroscopy SIMBAD [1][9]
아치스-F6 (WR 102ah in 아치스 성단) 101 25,000 15.75
(J 대역) 		33,900 Spectroscopy SIMBAD [29][30]
Sk -65° 47 (in NGC 1923 of LMC) 101 160,000 12.466 47,800 Evolution SIMBAD [22][13]
아치스-F1 (WR 102ad in 아치스 성단) 100.9 25,000 16.3
(J 대역) 		33,200 Spectroscopy SIMBAD [29][30]
Peony Star (WR 102ka in Peony Nebula near Galactic Center) 100 26,000 12.978
(J 대역) 		25,100 Spectroscopy SIMBAD [37][35]
VFTS 457 (in Tarantula Nebula of LMC) 100 164,000 13.74 39,800 Spectroscopy SIMBAD [5][2]
용골자리 에타 A (in 트럼플러 16 of 용골자리 성운) 100 7,500 4.3
(연성계 전체) 		9,400–35,200 Spectroscopy SIMBAD [38][39]
머서 30-1 A (WR 46-3 A in 머서 30 of Dragonfish Nebula) 99 40,000 10.33
(J 대역) 		32,200 Evolution SIMBAD [40][c][a]
Sk -68° 137 (in Tarantula Nebula of LMC) 99 160,000 13.346 50,000 Spectroscopy SIMBAD [12][13]
WR 25 A (in 트럼플러 16 of 용골자리 성운) 98 6,500 8.8
(연성계 전체) 		50,100 Evolution SIMBAD [27][9][a]
BI 253 (폭주성 from Tarantula Nebula of LMC) 97.6 164,000 13.76 54,000 Spectroscopy SIMBAD [11][41]
R136a8 (in Tarantula Nebula of LMC) 96 157,000 14.42 49,500 Evolution SIMBAD [18][42]
HD 38282 B (in Tarantula Nebula of LMC) 95 163,000 11.11
(연성계 전체) 		47,000 Binary SIMBAD [43][17]
HM 1-6 (in HM 1) 95 11,000 11.64 44,700 Evolution SIMBAD [20][44]
NGC 3603-42 (in HD 97950 of NGC 3603) 95 25,000 12.86 50,000 Spectroscopy SIMBAD [12][15]
R139 A (in Tarantula Nebula of LMC) 95 163,000 11.94
(연성계 전체) 		35,000 Binary SIMBAD [1][2]
BAT99-6 (in NGC 1747 of LMC) 94 165,000 11.95 56,000 Spectroscopy SIMBAD [1][13]
Sk -66° 172 (in N64 of LMC) 94 160,000 13.1 46,300 Spectroscopy SIMBAD [12][13][d]
ST2-22 (in NGC 2044 of LMC) 94 160,000 14.3 51,300 Evolution SIMBAD [22][45]
VFTS 259 (in Tarantula Nebula of LMC) 94 164,000 13.65 37,600 Spectroscopy SIMBAD [5][2]
VFTS 562 (in Tarantula Nebula of LMC) 94 164,000 13.66 42,200 Spectroscopy SIMBAD [5][2]
VFTS 512 (in Tarantula Nebula of LMC) 93 164,000 14.28 47,300 Spectroscopy SIMBAD [5][2]
HD 97950 A1b (WR 43a B in HD 97950 of NGC 3603) 92 24,800 11.18
(연성계 전체) 		40,000 Binary SIMBAD [14][15]
R136b (in Tarantula Nebula of LMC) 92 163,000 13.24 35,500 Evolution SIMBAD [18][2]
VFTS 16 (in Tarantula Nebula of LMC) 91.6 164,000 13.55 50,600 Spectroscopy SIMBAD [11][2]
HD 97950 A3 (in HD 97950 of NGC 3603) 91 24,800 12.95 50,000 Spectroscopy SIMBAD [12][15]
NGC 346-W1 (in NGC 346 of SMC) 91 200,000 12.57 43,400 Evolution SIMBAD [22][46]
웨스터하우트 49-2 (in 웨스터하우트 49) 90–240, 250±120 36,200 18.246
(J 대역) 		35,500 Spectroscopy SIMBAD [34][35]
R127 (in NGC 2055 of LMC) 90 160,000 10.15 10,000–27,000 Evolution SIMBAD [47][17]
VFTS 333 (in Tarantula Nebula of LMC) 90 164,000 12.49 37,600 Spectroscopy SIMBAD [5][2]
VFTS 267 (in [[타란툴라 성운] of LMC) 89 164,000 13.49 44,700 Spectroscopy SIMBAD [5][2]
VFTS 64 (in 타란툴라 성운 of LMC) 88 164,000 14.621 39,800 Spectroscopy SIMBAD [5][13]
BAT99-80 A (in NGC 2044 of LMC) 87 165,000 13
(연성계 전체) 		45,000 Spectroscopy SIMBAD [22][45]
R140b (in 타란툴라 성운 of LMC) 87 165,000 12.66 47,000 Spectroscopy SIMBAD [1][2]
VFTS 542 (in 타란툴라 성운 of LMC) 87 164,000 13.47 44,700 Spectroscopy SIMBAD [5][2]
VFTS 599 (in 타란툴라 성운 of LMC) 87 164,000 13.8 44,700 Spectroscopy SIMBAD [5][2]
WR 89 (in HM 1) 87 11,000 11.02 39,800 Evolution SIMBAD [27][17]
아치스-F7 (WR 102aj in 아치스 성단) 86.3 25,000 15.74
(J 대역) 		32,900 Spectroscopy SIMBAD [29][30]
Sk -69° 104 (in NGC 1910 of LMC) 86 160,000 12.1 39,900 Evolution SIMBAD [22][13]
VFTS 1017 (in 타란툴라 성운 of LMC) 86 164,000 14.5 50,100 Spectroscopy SIMBAD [5][2]
LH 10-3061 (in NGC 1763 of LMC) 85 160,000 13.491 52,000 Spectroscopy SIMBAD [12][13]
Sk 80 (in NGC 346 of SMC) 85 200,000 12.31 38,900 Evolution SIMBAD [22][48]
VFTS 603 (in 타란툴라 성운 of LMC) 85 164,000 13.99 42,200 Spectroscopy SIMBAD [5][2]
Sk -70° 91 (in BSDL 1830 of LMC) 84.09 165,000 12.78 48,900 Evolution SIMBAD [49][13][e]
R147 (in 타란툴라 성운 of LMC) 84 164,000 12.993 47,300 Spectroscopy SIMBAD [5][50]
HD 93250 A (in 트럼플러 16 of 용골자리 성운) 83.3 7,500 7.5
(연성계 전체) 		46,000 Evolution SIMBAD [51][9][a]
멜닉 33Na A (in 타란툴라 성운 of LMC) 83 163,000 13.79
(연성계 전체) 		50,000 Evolution SIMBAD [52][53]
WR 20a A (in 웨스터룬드 2) 82.7 20,000 13.28
(연성계 전체) 		43,000 Binary SIMBAD [54]
TIC 276934932 A (in NGC 2048 of LMC) 82 160,000 14.05
(연성계 전체) 		45,000 Spectroscopy SIMBAD [12][13]
WR 20a B (in 웨스터룬드 2) 81.9 20,000 13.28
(연성계 전체) 		43,000 Binary SIMBAD [54]
트럼플러 27-27 (in 트럼플러 27) 81 3,900 13.31 37,000 Evolution SIMBAD [20][17]
BAT99-96 (in Tarantula Nebula of LMC) 80 165,000 13.76 42,000 Spectroscopy SIMBAD [1][2]
HD 15570 (in IC 1805 of Heart Nebula) 80 7,500 8.11 46,000 Spectroscopy SIMBAD [8][9]
HD 38282 A (in Tarantula Nebula of LMC) 80 163,000 11.11
(연성계 전체) 		47,000 Binary SIMBAD [43][17]
HSH95-46 (in Tarantula Nebula of LMC) 80 163,000 14.56 47,500 Evolution SIMBAD [18][2]
아치스-F15 (in 아치스 성단) 79.7 25,000 16.12
(J 대역) 		35,600 Spectroscopy SIMBAD [29][30]
BI 237 (in BSDL 2527 of LMC) 79.66 165,000 13.83 51,300 Spectroscopy SIMBAD [49][13][f]
VFTS 94 (in Tarantula Nebula of LMC) 79 164,000 14.161 42,200 Spectroscopy SIMBAD [5][13]
VFTS 151 (in Tarantula Nebula of LMC) 79 164,000 14.13 42,200 Spectroscopy SIMBAD [5][2]
LH 41-32 (in NGC 1910 of LMC) 78 160,000 13.086 48,200 Evolution SIMBAD [22][13]
피스미스 24-17 (in 피스미스 24 of NGC 6357) 78 5,900 11.84 42,700 Spectroscopy SIMBAD [55][44]
VFTS 404 (in Tarantula Nebula of LMC) 78 164,000 14.14 44,700 Spectroscopy SIMBAD [5][2]
웨스터하우트 51-2 (in 웨스터하우트 51) 77 20,000 13.68
(J 대역) 		42,700 Evolution SIMBAD [6]
BAT99-68 (in BSDL 2505 of LMC) 76 165,000 14.13 45,000 Spectroscopy SIMBAD [1][13][g]
HD 93632 (in 콜린더 228 of 용골자리 성운) 76 10,000 8.23 45,400 Evolution SIMBAD [20][9]
NGC 346-W3 (in NGC 346 of SMC) 76 200,000 12.8 52,500 Evolution SIMBAD [22][46]
VFTS 169 (in Tarantula Nebula of LMC) 76 164,000 14.437 47,300 Spectroscopy SIMBAD [5][13]
VFTS 440 (in Tarantula Nebula of LMC) 76 164,000 12.046 39,800 Spectroscopy SIMBAD [5][13]
AB1 (in DEM S10 of SMC) 75 197,000 15.238 79,000 Spectroscopy SIMBAD [56][46][h]
WR 22 A (in Bochum 10 of 용골자리 성운) 75 8,300 6.42
(연성계 전체) 		44,700 Evolution SIMBAD [27][9][i]
피스미스 24-1NE (in 피스미스 24 of NGC 6357) 74 6,500 11 42,500 Binary SIMBAD [55][57]
VFTS 608 (in Tarantula Nebula of LMC) 74 164,000 14.22 42,200 Spectroscopy SIMBAD [5][2]
HSH95-31 (in Tarantula Nebula of LMC) 73 163,000 14.12 47,500 Evolution SIMBAD [18][2]
머서 30-3 (in 머서 30 of Dragonfish Nebula) 73 40,000 12.62
(J 대역) 		39,300 Evolution SIMBAD [40][c]
머서 30-11 (in 머서 30 of Dragonfish Nebula) 73 40,000 12.33
(J 대역) 		36,800 Evolution SIMBAD [40][c]
VFTS 566 (in Tarantula Nebula of LMC) 73 164,000 14.05 44,700 Spectroscopy SIMBAD [5][2]
LH 64-16 (in NGC 2001 of LMC) 72 160,000 13.666 50,900 Evolution SIMBAD [22][24]
NGC 2044-W35 (in NGC 2044 of LMC) 72 160,000 14.1 48,200 Evolution SIMBAD [22][13]
VFTS 216 (in Tarantula Nebula of LMC) 72 164,000 14.389 44,700 Spectroscopy SIMBAD [5][13]
ST2-1 (in NGC 2044 of LMC) 71 160,000 14.3 44,100 Evolution SIMBAD [22][45]
VFTS 3 (in 타란툴라 성운 of LMC) 71 164,000 11.56 21,000 Spectroscopy SIMBAD [58][2]
아치스-F12 (WR 102af in 아치스 성단) 70 25,000 16.4
(J 대역) 		36,900 Spectroscopy SIMBAD [29][30]
HD 15629 (in IC 1805 of Heart Nebula) 70 7,500 8.42 45,900 Spectroscopy SIMBAD [8][9]
HD 37974 (in N135 of LMC) 70 163,000 10.99 22,500 Spectroscopy SIMBAD [59][17][j]
HD 93129 Ab (in 트럼플러 14 of 용골자리 성운) 70 7,500 7.31
(연성계 전체) 		44,000 Trinary SIMBAD [33][60]
M33 X-7 B (in Triangulum Galaxy) 70 2,700,000 18.7 35,000 Binary SIMBAD [61][62]
Sk -69° 194 A (in NGC 2033 of LMC) 70 160,000 12.131
(연성계 전체) 		45,000 Evolution SIMBAD [22][50][a]
VFTS 125 (in 타란툴라 성운 of LMC) 69.6 164,000 16.6 55,200 Spectroscopy SIMBAD [11][45]
HD 46150 (in NGC 2244 of Rosette Nebula) 69 5,200 6.73 44,000 Spectroscopy SIMBAD [12][9]
HD 229059 (in Berkeley 87) 69 3,000 8.7 26,300 Evolution SIMBAD [20][9]
ST2-3 (in NGC 2044 of LMC) 69 160,000 14.264 44,900 Evolution SIMBAD [22][13]
ST2-32 (in NGC 2044 of LMC) 69 160,000 13.903 45,400 Evolution SIMBAD [22][13]
W28-23 (in NGC 2033 of LMC) 69 160,000 13.702 51,300 Evolution SIMBAD [22][24]
HD 93403 A (in 트럼플러 16 of 용골자리 성운) 68.5 10,400 8.27
(연성계 전체) 		39,300 Binary SIMBAD [63][17]
HD 93130 (in 콜린더 228 of 용골자리 성운) 68 10,000 8.04 39,900 Evolution SIMBAD [20][9]
HM 1-8 (in HM 1) 68 11,000 12.52 46,100 Evolution SIMBAD [20][44]
HSH95-47 (in 타란툴라 성운 of LMC) 68 163,000 14.72 43,500 Evolution SIMBAD [18][2]
HSH95-48 (in 타란툴라 성운 of LMC) 68 163,000 14.75 46,500 Evolution SIMBAD [18][42]
웨스터하우트 51-61 (in 웨스터하우트 51) 68 20,000 18.16
(J 대역) 		38,000 Evolution SIMBAD [6][35]
BAT99-93 (in 타란툴라 성운 of LMC) 67 165,000 13.446 45,000 Spectroscopy SIMBAD [1][13]
Sk -69° 200 (in NGC 2033 of LMC) 67 160,000 11.18 26,300 Evolution SIMBAD [22][13]
아치스-F18 (in 아치스 성단) 66.9 25,000 16.7
(J 대역) 		36,900 Spectroscopy SIMBAD [29][30]
아치스-F4 (WR 102al in 아치스 성단) 66.4 25,000 15.63
(J 대역) 		36,800 Spectroscopy SIMBAD [29][30]
BAT99-59 A (in NGC 2020 of LMC) 66 165,000 13.186
(연성계 전체) 		71,000 Spectroscopy SIMBAD [1][13][a]
BAT99-104 (in 타란툴라 성운 of LMC) 66 165,000 12.5 63,000 Spectroscopy SIMBAD [1][13]
HD 5980 B (in NGC 346 of SMC) 66 200,000 11.31
(연성계 전체) 		45,000 Trinary SIMBAD [64][60]
HD 190429 A (near Barnard 146) 66 7,800 6.63
(연성계 전체) 		46,000 Binary SIMBAD [65][9]
LH 31-1003 (in NGC 1858 of LMC) 66 160,000 13.186 41,900 Evolution SIMBAD [22][13]
LH 114-7 (in N70 of LMC) 66 160,000 13.66 50,000 Spectroscopy SIMBAD [12][13][k]
피스미스 24-1SW (in 피스미스 24 of NGC 6357) 66 6,500 11.1 40,000 Binary SIMBAD [55][57]
BAT99-126 (in NGC 2081 of LMC) 65 165,000 13.166 71,000 Spectroscopy SIMBAD [1][13]
HSH95-40 (in Tarantula Nebula of LMC) 65 163,000 14.56 47,500 Evolution SIMBAD [18][2]
HSH95-58 (in Tarantula Nebula of LMC) 65 163,000 14.8 47,500 Evolution SIMBAD [18][2]
HSH95-89 (in Tarantula Nebula of LMC) 65 163,000 14.76 44,000 Spectroscopy SIMBAD [42]
VFTS 63 (in Tarantula Nebula of LMC) 65 164,000 14.4 42,200 Spectroscopy SIMBAD [5][45]
VFTS 145 (in Tarantula Nebula of LMC) 65 164,000 14.3 39,800 Spectroscopy SIMBAD [5][2]
VFTS 518 (in Tarantula Nebula of LMC) 65 164,000 15.11 44,700 Spectroscopy SIMBAD [5][2]
웨스터하우트 49-8 (in 웨스터하우트 49) 65 36,200 15.617
(J 대역) 		40,700 Evolution SIMBAD [34][35]
BD+43° 3654 (폭주성 from 백조자리 OB2) 64.6 5,400 10.06 40,400 Evolution SIMBAD [66][60]
BAT99-129 A (in DEM L294 of LMC) 64 165,000 14.701
(연성계 전체) 		79,000 Spectroscopy SIMBAD [1][13][l][a]
HSH95-50 (in Tarantula Nebula of LMC) 64 163,000 14.65 47,000 Evolution SIMBAD [18][2]
Sk -69° 25 (in NGC 1748 of LMC) 64 160,000 11.886 43,600 Evolution SIMBAD [22][13]
트럼플러 27-23 (in 트럼플러 27) 64 3,900 10.09 27,500 Evolution SIMBAD [20][17]
웨스터하우트 49-5 (in 웨스터하우트 49) 64 36,200 15.623
(J 대역) 		42,700 Evolution SIMBAD [34][35]
HD 46223 (in NGC 2244 of Rosette Nebula) 63 5,200 7.28 46,000 Spectroscopy SIMBAD [12][9]
HD 64568 (in NGC 2467 of Puppis OB2) 63 16,000 9.39 54,000 Spectroscopy SIMBAD [12][17]
HD 303308 (in 트럼플러 16 of 용골자리 성운) 63 9,200 8.17 51,300 Evolution SIMBAD [20][17]
HR 6187 A (in NGC 6193 of Ara OB1) 63 4,300 5.54
(연성계 전체) 		46,500 Septenary SIMBAD [67][9]
LH 10-3058 (in NGC 1763 of LMC) 63 160,000 14.089 54,000 Spectroscopy SIMBAD [12][13]
ST5-71 (in NGC 2074 of LMC) 63 160,000 13.266 45,400 Evolution SIMBAD [22][13]
AB9 (in DEM S80 of SMC) 62 197,000 15.431 100,000 Spectroscopy SIMBAD [56][46][m]
Brey 32 B (in NGC 1966 of LMC) 62 165,000 12.32
(연성계 전체) 		43,600 Evolution SIMBAD [22][17]
HD 93160 (in 트럼플러 14 of 용골자리 성운) 62 8,000 7.6 42,700 Evolution SIMBAD [20][9]
HSH95-35 (in Tarantula Nebula of LMC) 62 163,000 14.43 47,500 Evolution SIMBAD [18][2]
LH 41-1017 (in NGC 1910 of LMC) 62 160,000 12.266 42,700 Evolution SIMBAD [22][13]
머서 30-6a A (WR 46-4 A in 머서 30 of Dragonfish Nebula) 62 40,000 10.39
(J 대역) 		29,900 Evolution SIMBAD [40][c][a]
ST4-18 (in NGC 2081 of LMC) 62 160,000 13.639 44,800 Evolution SIMBAD [22][13]
VFTS 664 (in Tarantula Nebula of LMC) 62 164,000 13.937 39,900 Spectroscopy SIMBAD [5][13]
HD 229196 (in 백조자리 OB9) 61.6 5,000 8.59 40,900 Evolution SIMBAD [66][44]
AB8 B (in NGC 602 of SMC) 61 197,000 12.83
(연성계 전체) 		45,000 Binary SIMBAD [64][68]
BAT99-79 A (in NGC 2044 of LMC) 61 165,000 13.486
(연성계 전체) 		42,000 Spectroscopy SIMBAD [1][13][a]
HD 5980 A (in NGC 346 of SMC) 61 200,000 11.31
(연성계 전체) 		21,000–53,000 Trinary SIMBAD [64][60]
LH 41-18 (in NGC 1910 of LMC) 61 160,000 12.586 38,500 Evolution SIMBAD [22][13]
머서 30-9 A (in 머서 30 of Dragonfish Nebula) 61 40,000 12.25
(J 대역) 		34,500 Evolution SIMBAD [40][c][a]
ST5-25 (in NGC 2074 of LMC) 61 160,000 13.551 48,600 Evolution SIMBAD [22][24]
VFTS 422 (in Tarantula Nebula of LMC) 61 164,000 15.14 39,800 Spectroscopy SIMBAD [5][2]
WR 102hb (in 다섯쌍둥이 성단) 61 26,000 13.9
(J 대역) 		25,100 Evolution SIMBAD [69][70]
Sk -67° 166 (in GKK-A144 of LMC) 60.68 160,000 12.22 41,800 Spectroscopy SIMBAD [49][13][n]
Sk -67° 167 (in GKK-A144 of LMC) 60.68 160,000 12.586 41,800 Spectroscopy SIMBAD [49][13][n]
Sk -71° 46 (in BSDL 2242 of LMC) 60.68 160,000 13.241 41,800 Spectroscopy SIMBAD [49][13][o]
Brey 10 (in NGC 1770 of LMC) 60 165,000 12.69 117,000 Evolution SIMBAD [22][17]
Brey 94 A (in NGC 2081 of LMC) 60 165,000 12.996
(연성계 전체) 		83,000 Evolution SIMBAD [22][13][a]
Brey 95a A (in NGC 2081 of LMC) 60 165,000 12.2
(연성계 전체) 		83,000 Evolution SIMBAD [22][71][a]
HSH95-55 (in Tarantula Nebula of LMC) 60 163,000 14.74 47,500 Evolution SIMBAD [18][2]
머서 30-7 A (WR 46-5 A in 머서 30 of Dragonfish Nebula) 60 40,000 11.516
(J 대역) 		41,400 Evolution SIMBAD [40][c][a]
R134 (in Tarantula Nebula of LMC) 60 164,000 12.75 39,800 Spectroscopy SIMBAD [5][2]
R142 (in Tarantula Nebula of LMC) 60 164,000 11.82 18,000 Spectroscopy SIMBAD [58][2]
R143 (in Tarantula Nebula of LMC) 60 160,000 12.014 18,000–36,000 Evolution SIMBAD [47][13]
Sk -69° 142a (in NGC 1983 of LMC) 60 160,000 11.093 34,000 Evolution SIMBAD [47][50]
Sk -69° 259 (in NGC 2081 of LMC) 60 160,000 11.93 23,000 Evolution SIMBAD [22][17]
Var 83 (in Triangulum Galaxy) 60 3,000,000 16.027 18,000–37,000 Evolution SIMBAD [72][73]
VFTS 430 (in Tarantula Nebula of LMC) 60 164,000 15.11 24,500 Spectroscopy SIMBAD [58][2]
아치스-F14 54–65
WR 102ea[74] 58
백조자리 OB2-11 58
아치스-F3 52–63
남십자자리 CD A + B[75] A=57, B=48
아치스-B1 50–60
플라스켓의 별 A=54, B=56
BD+40° 4210 54
HD 93129 B[76] 52
백조자리 OB2-4 52
아치스-F20 47–57
아치스-F16 46–56
WR102c[77] 45–55
아치스-F8 43–51
NGC 3603 내 셰어 25 40–52
아치스-F2 42–49
황새치자리 S 45
IRS-8*[78] 44.5
백조자리 OB2-8A 44 + 37
백조자리 OB2-1 44
기린자리 알파 43
피스미스 24-2 43
오리온자리 키² 42.3
백조자리 OB2-6 42
오리온자리 엡실론 40
세페우스자리 RW 40
오리온자리 세타1 C 40
나오스 22.5-56.6
NGC 300 X-1의 짝별[79] 38
피스미스 24-16 38
피스미스 24-25 38
전갈자리 제타1 36
피스미스 24-13 35
백조자리 OB2-5 31 + 9
IC 10 X-1의 짝별[80] 35
아치스-F5 31–36
백조자리 OB2-18 33
오리온자리 제타 33
세페우스자리 19 30–35
페르세우스자리 크시 26–36
돛자리 감마 A 30
백조자리 P 30
IRS 15[81] 26
카시오페이아자리 6[82] 25
피스미스 24-3 25
백조자리 KY 25
NGC 7538 S[83] 25
카시오페이아자리 로 14-30
범례
볼프-레이에별
O형 항성
B형 항성
LBV
극대거성

참고 문헌

  1. ↑ 가 나 다 라 마 바 사 아 자 차 카 타 파 하 Hainich, R.; Rühling, U.; Todt, H.; Oskinova, L. M.; Liermann, A.; Gräfener, G.; 외. (May 2014). “The Wolf-Rayet stars in the Large Magellanic Cloud. A comprehensive analysis of the WN class”. 《Astronomy & Astrophysics》 565: A27. arXiv:1401.5474. Bibcode:2014A&A...565A..27H. doi:10.1051/0004-6361/201322696. ISSN 0004-6361. S2CID 55123954. 
  2. ↑ 가 나 다 라 마 바 사 아 자 차 카 타 파 하 거 너 더 러 머 버 서 어 저 처 커 터 퍼 허 고 노 도 로 모 보 소 오 조 초 코 토 포 호 구 누 두 루 무 부 수 우 주 추 Doran, E.I.; Crowther, P.A.; de Koter, A.; Evans, C.J.; McEvoy, C.; Walborn, N.R.; 외. (October 2013). “The VLT-FLAMES Tarantula Survey: XI. A census of the hot luminous stars and their feedback in 30 Doradus”. 《Astronomy & Astrophysics》 558: A134. arXiv:1308.3412. Bibcode:2013A&A...558A.134D. doi:10.1051/0004-6361/201321824. ISSN 0004-6361. S2CID 118510909. 
  3. ↑ 가 나 다 Bestenlehner, Joachim M.; Crowther, Paul A.; Caballero-Nieves, Saida M.; Schneider, Fabian R. N.; Simón-Díaz, Sergio; Brands, Sarah A.; de Koter, Alex; Gräfener, Götz; Herrero, Artemio; Langer, Norbert; Lennon, Daniel J. (2020년 12월 1일). “The R136 star cluster dissected with Hubble Space Telescope/STIS - II. Physical properties of the most massive stars in R136”. 《Monthly Notices of the Royal Astronomical Society》 499 (2): 1918–1936. arXiv:2009.05136. Bibcode:2020MNRAS.499.1918B. doi:10.1093/mnras/staa2801. ISSN 0035-8711. 
  4. ↑ 가 나 다 Kalari, Venu M.; Horch, Elliott P.; Salinas, Ricardo; Vink, Jorick S.; Andersen, Morten; Bestenlehner, Joachim M.; Rubio, Monica (2022년 7월 26일). “Resolving the Core of R136 in the Optical”. 《The Astrophysical Journal》 935 (2): 162. arXiv:2207.13078. Bibcode:2022ApJ...935..162K. doi:10.3847/1538-4357/ac8424. S2CID 251067072. 
  5. ↑ 가 나 다 라 마 바 사 아 자 차 카 타 파 하 거 너 더 러 머 버 서 어 저 처 커 터 퍼 허 고 노 도 로 Bestenlehner, J.M.; Gräfener, G.; Vink, J.S.; Najarro, F.; de Koter, A.; Sana, H.; 외. (October 2014). “The VLT-FLAMES Tarantula Survey: XVII. Physical and wind properties of massive stars at the top of the main sequence”. 《Astronomy & Astrophysics》 570: A38. arXiv:1407.1837. Bibcode:2014A&A...570A..38B. doi:10.1051/0004-6361/201423643. ISSN 0004-6361. S2CID 118606369. 
  6. ↑ 가 나 다 라 마 Bik, A.; Henning, Th.; Wu, S.-W.; Zhang, M.; Brandner, W.; Pasquali, A.; Stolte, A. (April 2019). “Near-infrared spectroscopy of the massive stellar population of W51: evidence for multi-seeded star formation”. 《Astronomy & Astrophysics》 624: A63. arXiv:1902.05460. Bibcode:2019A&A...624A..63B. doi:10.1051/0004-6361/201935061. ISSN 0004-6361. S2CID 118711844. 
  7. ↑ 가 나 Bagnulo, S.; Wade, G.A.; Nazé, Y.; Grunhut, J.H.; Shultz, M.E.; Asher, D.J.; 외. (March 2020). “A search for strong magnetic fields in massive and very massive stars in the Magellanic Clouds”. 《Astronomy & Astrophysics》 635: A163. arXiv:2002.12061. Bibcode:2020A&A...635A.163B. doi:10.1051/0004-6361/201937098. ISSN 0004-6361. S2CID 211532767. 
  8. ↑ 가 나 다 De Becker, M.; Rauw, G.; Manfroid, J.; Eenens, P. (September 2006). “Early-type stars in the young open cluster IC 1805: II. The probably single stars HD 15570 and HD 15629, and the massive binary/triple system HD 15558”. 《Astronomy & Astrophysics》 456 (3): 1121–1130. arXiv:astro-ph/0606379. Bibcode:2006A&A...456.1121D. doi:10.1051/0004-6361:20065300. ISSN 0004-6361. S2CID 16519684. 
  9. ↑ 가 나 다 라 마 바 사 아 자 차 카 타 파 하 거 너 더 Ducati, J.R. (2002). VizieR Online Data Catalog: Catalogue of Stellar Photometry in Johnson's 11-color system (보고서). Collection of Electronic Catalogues 2237. CDS/ADC. Bibcode:2002yCat.2237....0D. S2CID 118191108. 
  10. ↑ 가 나 Tehrani, Katie A.; Crowther, Paul A.; Bestenlehner, Joachim M.; Littlefair, Stuart P.; Pollock, A.M.T.; Parker, Richard J.; Schnurr, Olivier (2019년 4월 1일). “Weighing Melnick 34: the most massive binary system known”. 《Monthly Notices of the Royal Astronomical Society》 484 (2): 2692–2710. arXiv:1901.04769. Bibcode:2019MNRAS.484.2692T. doi:10.1093/mnras/stz147. ISSN 0035-8711. S2CID 119069481. 
  11. ↑ 가 나 다 라 Schneider, F.R.N.; Sana, H.; Evans, C.J.; Bestenlehner, J.M.; Castro, N.; Fossati, L.; 외. (2018년 1월 5일). “An excess of massive stars in the local 30 Doradus starburst”. 《Science》 (영어) 359 (6371): 69–71. arXiv:1801.03107. Bibcode:2018Sci...359...69S. doi:10.1126/science.aan0106. ISSN 0036-8075. PMID 29302009. S2CID 206658504. 
  12. ↑ 가 나 다 라 마 바 사 아 자 차 카 타 Walborn, Nolan R.; Howarth, Ian D.; Lennon, Daniel J.; Massey, Philip; Oey, M. S.; Moffat, Anthony F. J.; 외. (May 2002). “A New Spectral Classification System for the Earliest O Stars: Definition of Type O2”. 《The Astronomical Journal》 123 (5): 2754–2771. Bibcode:2002AJ....123.2754W. doi:10.1086/339831. ISSN 0004-6256. S2CID 122127697. 
  13. ↑ 가 나 다 라 마 바 사 아 자 차 카 타 파 하 거 너 더 러 머 버 서 어 저 처 커 터 퍼 허 고 노 도 로 모 보 소 오 조 초 코 토 포 호 Bonanos, A.Z.; Massa, D.L.; Sewilo, M.; Lennon, D.J.; Panagia, N.; Smith, L.J.; 외. (2009년 10월 1일). “Spitzer SAGE Infrared Photometry of Massive Stars in the Large Magellanic Cloud”. 《The Astronomical Journal》 138 (4): 1003–1021. arXiv:0905.1328. Bibcode:2009AJ....138.1003B. doi:10.1088/0004-6256/138/4/1003. ISSN 0004-6256. S2CID 14056495. 
  14. ↑ 가 나 다 라 Crowther, Paul A.; Schnurr, Olivier; Hirschi, Raphael; Yusof, Norhasliza; Parker, Richard J.; Goodwin, Simon P.; Kassim, Hasan Abu (2010년 10월 21일). “The R136 star cluster hosts several stars whose individual masses greatly exceed the accepted 150 M⊙ stellar mass limit”. 《Monthly Notices of the Royal Astronomical Society》 (영어) 408 (2): 731–751. arXiv:1007.3284. Bibcode:2010MNRAS.408..731C. doi:10.1111/j.1365-2966.2010.17167.x. ISSN 0035-8711. S2CID 53001712. 
  15. ↑ 가 나 다 라 마 바 Melena, Nicholas W.; Massey, Philip; Morrell, Nidia I.; Zangari, Amanda M. (2008년 3월 1일). “The massive star content of NGC 3603”. 《The Astronomical Journal》 135 (3): 878–891. arXiv:0712.2621. Bibcode:2008AJ....135..878M. doi:10.1088/0004-6256/135/3/878. ISSN 0004-6256. S2CID 16765414. 
  16. ↑ Evans, C.J.; Walborn, N.R.; Crowther, P.A.; Hénault-Brunet, V.; Massa, D.; Taylor, W.D.; 외. (2010년 6월 1일). “A massive runaway star from 30 Doradus”. 《The Astrophysical Journal》 715 (2): L74–L79. arXiv:1004.5402. Bibcode:2010ApJ...715L..74E. doi:10.1088/2041-8205/715/2/L74. ISSN 2041-8205. S2CID 118498849. 
  17. ↑ 가 나 다 라 마 바 사 아 자 차 카 타 파 하 거 Zacharias, N.; Finch, C.T.; Girard, T.M.; Henden, A.; Bartlett, J.L.; Monet, D.G.; Zacharias, M.I. (July 2012). “VizieR On-Line Data Catalog: UCAC4 Catalogue”. 《VizieR On-Line Data Catalog: I/322A. Originally Published in: 2012yCat.1322....0Z; 2013AJ....145...44Z》 1322. Bibcode:2012yCat.1322....0Z. S2CID 211646126. 
  18. ↑ 가 나 다 라 마 바 사 아 자 차 카 타 파 하 거 너 Brands, S.; de Koter, A.; Bestenlehner, J.; Crowther, P.; Sundqvist, J.; Puls, J.; 외. (2022년 4월 7일). “The R136 star cluster dissected with Hubble Space Telescope/STIS. III. The most massive stars and their clumped winds”. 《Astronomy & Astrophysics》 663: A36. arXiv:2202.11080. Bibcode:2022A&A...663A..36B. doi:10.1051/0004-6361/202142742. ISSN 0004-6361. S2CID 247025548. 
  19. ↑ Roman-Lopes, A.; Franco, G.A.P.; Sanmartim, D. (2016년 5월 26일). “SOAR Optical and Near-infrared Spectroscopic Survey of Newly Discovered Massive Stars in the Periphery of Galactic Massive Star Clusters I-NGC 3603”. 《The Astrophysical Journal》 823 (2): 96. arXiv:1604.01096. Bibcode:2016ApJ...823...96R. doi:10.3847/0004-637X/823/2/96. ISSN 1538-4357. S2CID 119204619. 
  20. ↑ 가 나 다 라 마 바 사 아 자 차 카 Massey, Philip; DeGioia-Eastwood, Kathleen; Waterhouse, Elizabeth (February 2001). “The progenitor masses of Wolf-Rayet stars and luminous blue variables determined from cluster turnoffs. II. Results from 12 galactic clusters and OB associations”. 《The Astronomical Journal》 121 (2): 1050–1070. arXiv:astro-ph/0010654. Bibcode:2001AJ....121.1050M. doi:10.1086/318769. ISSN 0004-6256. S2CID 53345173. 
  21. ↑ Vázquez, R.A.; Baume, G. (June 2001). “The open cluster Havlen-Moffat no. 1 revisited”. 《Astronomy & Astrophysics》 371 (3): 908–920. Bibcode:2001A&A...371..908V. doi:10.1051/0004-6361:20010410. ISSN 0004-6361. S2CID 121918776. 
  22. ↑ 가 나 다 라 마 바 사 아 자 차 카 타 파 하 거 너 더 러 머 버 서 어 저 처 커 터 퍼 허 고 노 도 Massey, Philip; Waterhouse, Elizabeth; DeGioia-Eastwood, Kathleen (May 2000). “The progenitor masses of Wolf-Rayet stars and luminous blue variables determined from cluster turnoffs. I. Results from 19 OB associations in the Magellanic Clouds”. 《The Astronomical Journal》 119 (5): 2214–2241. arXiv:astro-ph/0002233. Bibcode:2000AJ....119.2214M. doi:10.1086/301345. ISSN 0004-6256. S2CID 16891188. 
  23. ↑ Fabricius, C.; Høg, E.; Makarov, V.V.; Mason, B.D.; Wycoff, G.L.; Urban, S.E. (March 2002). “The Tycho double star catalogue”. 《Astronomy & Astrophysics》 384 (1): 180–189. Bibcode:2002A&A...384..180F. doi:10.1051/0004-6361:20011822. ISSN 0004-6361. S2CID 56060737. 
  24. ↑ 가 나 다 라 Zaritsky, Dennis; Harris, Jason; Thompson, Ian B.; Grebel, Eva K. (October 2004). “The Magellanic Clouds Photometric Survey: The Large Magellanic Cloud Stellar Catalog and Extinction Map”. 《The Astronomical Journal》 (영어) 128 (4): 1606–1614. arXiv:astro-ph/0407006. Bibcode:2004AJ....128.1606Z. doi:10.1086/423910. ISSN 0004-6256. S2CID 119532934. 
  25. ↑ Drew, J.E.; Herrero, A.; Mohr-Smith, M.; Monguió, M.; Wright, N.J.; Kupfer, T.; Napiwotzki, R. (2018년 10월 21일). “Massive stars in the hinterland of the young cluster, Westerlund 2”. 《Monthly Notices of the Royal Astronomical Society》 480 (2): 2109–2124. arXiv:1807.06486. Bibcode:2018MNRAS.480.2109D. doi:10.1093/mnras/sty1905. ISSN 0035-8711. S2CID 53126230. 
  26. ↑ Vargas Álvarez, Carlos A.; Kobulnicky, Henry A.; Bradley, David R.; Kannappan, Sheila J.; Norris, Mark A.; Cool, Richard J.; Miller, Brendan P. (2013년 3월 25일). “The distance to the massive galactic cluster Westerlund 2 from a spectroscopic and HST photometric study”. 《The Astronomical Journal》 145 (5): 125. arXiv:1302.0863. Bibcode:2013AJ....145..125V. doi:10.1088/0004-6256/145/5/125. ISSN 0004-6256. S2CID 67769122. 
  27. ↑ 가 나 다 라 Hamann, W.-R.; Gräfener, G.; Liermann, A.; Hainich, R.; Sander, A.a.C.; Shenar, T.; 외. (2019년 5월 1일). “The galactic WN stars revisited - impact of Gaia distances on fundamental stellar parameters”. 《Astronomy & Astrophysics》 (영어) 625: A57. arXiv:1904.04687. Bibcode:2019A&A...625A..57H. doi:10.1051/0004-6361/201834850. ISSN 0004-6361. S2CID 104292503. 
  28. ↑ Samus, N.N.; Kazarovets, E.V.; Durlevich, O.V.; Kireeva, N.N.; Pastukhova, E.N. (January 2009). “VizieR Online Data Catalog: General Catalogue of Variable Stars (Samus+ 2007-2013)”. 《VizieR On-Line Data Catalog: B/GCVS. Originally Published in: 2017ARep...61...80S; 2017AZh....94...87S》 1. Bibcode:2009yCat....102025S. S2CID 208116145. 
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  59. ↑ Kastner, Joel H.; Buchanan, Catherine L.; Sargent, B.; Forrest, W. J. (2006년 2월 10일). “Spitzer Spectroscopy of Dusty Disks around B[e] Hypergiants in the Large Magellanic Cloud”. 《The Astrophysical Journal》 (영어) 638 (1): L29–L32. Bibcode:2006ApJ...638L..29K. doi:10.1086/500804. ISSN 0004-637X. S2CID 121769413. 
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  62. ↑ Grimm, H.-J.; McDowell, J.; Zezas, A.; Kim, D.-W.; Fabbiano, G. (December 2005). “The X-Ray Binary Population in M33. I. Source List and Luminosity Function”. 《The Astrophysical Journal Supplement Series》 (영어) 161 (2): 271–303. arXiv:astro-ph/0506353. Bibcode:2005ApJS..161..271G. doi:10.1086/468185. ISSN 0067-0049. S2CID 119381693. 
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  75. ↑ Bhatt, H.; Pandey, J. C.; Kumar, B.; Singh, K. P.; Sagar, R. (2010). “X-ray emission characteristics of two Wolf-Rayet binaries: V444 Cyg and CD Cru”. 《Monthly Notices of the Royal Astronomical Society》 402 (3): 1767. arXiv:0911.1489. Bibcode:2010MNRAS.402.1767B. doi:10.1111/j.1365-2966.2009.15999.x. 
  76. ↑ Vink, J. S.; Davies, B.; Harries, T. J.; Oudmaijer, R. D.; Walborn, N. R. (2009). “On the presence and absence of disks around O-type stars”. 《Astronomy and Astrophysics》 505 (2): 743. arXiv:0909.0888. Bibcode:2009A&A...505..743V. doi:10.1051/0004-6361/200912610. 
  77. ↑ 인용 오류: <ref> 태그가 잘못되었습니다; barniske라는 이름을 가진 주석에 텍스트가 없습니다
  78. ↑ Geballe, T. R.; Najarro, F.; Rigaut, F.; Roy, J. ‐R. (2006). “TheK‐Band Spectrum of the Hot Star in IRS 8: An Outsider in the Galactic Center?”. 《The Astrophysical Journal》 652: 370. arXiv:astro-ph/0607550. Bibcode:2006ApJ...652..370G. doi:10.1086/507764. 
  79. ↑ Paul A Crowther; Carpano; Hadfield; Pollock (2007). “On the optical counterpart of NGC300 X-1 and the global Wolf-Rayet content of NGC300”. 《Astronomy and Astrophysics》 469 (31): L31. arXiv:0705.1544. Bibcode:2007A&A...469L..31C. doi:10.1051/0004-6361:20077677. 
  80. ↑ Bulik, T.; Belczynski, K.; Prestwich, A. (2011). “Ic10 X-1/ngc300 X-1: The Very Immediate Progenitors of Bh-Bh Binaries”. 《The Astrophysical Journal》 730 (2): 140. doi:10.1088/0004-637X/730/2/140. 
  81. ↑ Chini, R.; Hoffmeister, V. H.; Nielbock, M.; Scheyda, C. M.; Steinacker, J.; Siebenmorgen, R.; Nürnberger, D. (2006). “A Remnant Disk around a Young Massive Star”. 《The Astrophysical Journal》 645: L61. doi:10.1086/505862. 
  82. ↑ Achmad, L.; Lamers, H. J. G. L. M.; Pasquini, L. (1997). “Radiation driven wind models for A, F and G supergiants”. 《Astronomy and Astrophysics》 320: 196. Bibcode:1997A&A...320..196A. 
  83. ↑ Moscadelli, L.; Goddi, C. (2014). “A multiple system of high-mass YSOs surrounded by disks in NGC 7538 IRS1”. 《Astronomy & Astrophysics》 566: A150. doi:10.1051/0004-6361/201423420. 

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인용 오류: "lower-alpha"이라는 이름을 가진 그룹에 대한 <ref> 태그가 존재하지만, 이에 대응하는 <references group="lower-alpha" /> 태그가 없습니다

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