{{위키데이터 속성 추적}}
아래 목록은 관측된 별들 중 '''[[유효온도]]가 높은 별'''들을 순서대로 정렬한 것으로 단위는 [[켈빈]]이다. 유효온도가 60,000[[켈빈|K]]보다 높은 별이 포함되며 [[밀집성]]은 제외된다.

==목록==
{| class="wikitable sortable"
! 항성 이름
! [[유효온도]]<br>([[켈빈|K]])
! [[질량]]<br>({{태양질량|link=y}})
! [[광도 (천문학)|복사광도]]<br>({{태양광도|link=y}})
! [[항성분류|분광형]]
! 대략 태양계로부터의 거리<br>{{nowrap|([[광년]])}}
! 참고문헌
|-
|[[WR 102]]
|200,000
|16.1
|380,000
|[[볼프-레이에별|WO2]]
|8,610<ref name=":1" />
|<ref name=sander>{{저널 인용 | last1 = Sander | first1 = A. | last2 = Hamann | first2 = W. -R. | last3 = Todt | first3 = H. | title = The Galactic WC stars | doi = 10.1051/0004-6361/201117830 | journal = Astronomy & Astrophysics | volume = 540 | pages = A144 | year = 2012 |arxiv = 1201.6354 |bibcode = 2012A&A...540A.144S | s2cid = 119182468 }}</ref><ref name=":0">{{저널 인용|last1=Sander|first1=A. A. C.|last2=Hamann|first2=W.-R.|last3=Todt|first3=H.|last4=Hainich|first4=R.|last5=Shenar|first5=T.|last6=Ramachandran|first6=V.|last7=Oskinova|first7=L. M.|date=2019-01-01|title=The Galactic WC and WO stars. The impact of revised distances from Gaia DR2 and their role as massive black hole progenitors|bibcode=2019A&A...621A..92S|journal=Astronomy and Astrophysics|volume=621|pages=A92|doi=10.1051/0004-6361/201833712|arxiv=1807.04293|issn=0004-6361|doi-access=free}}</ref>
|-
|[[WR 142]]
|200,000
|28.6
|912,000
|[[볼프-레이에별|WO2]]
|5,400
|<ref name=":0" />
|-
|[[LMC195-1]]
|200,000
|
|257,000
|[[볼프-레이에별|WO2]]
|160,000
|<ref name=wo>{{저널 인용| doi = 10.1088/0004-637X/788/1/83 | title=A modern search for Wolf–Rayet stars in the Magellanic Clouds: First results | journal=The Astrophysical Journal | date=2014 | volume=788 | issue=1 | pages=83 | first=Philip | last=Massey| bibcode=2014ApJ...788...83M |arxiv = 1404.7441 | s2cid=119177379 }}</ref>
|-
|[[BAT99-123]]
|170,000
|
|158,000
|[[볼프-레이에별|WO3]]
|~160,000
|<ref name=tramper/>
|-
|[[WR 93b]]
|160,000
|8.1
|110,000
|[[볼프-레이에별|WO3]]
|7,470<ref name=":1">{{웹 인용|title=Wolf-Rayet Star Catalogue|url=http://pacrowther.staff.shef.ac.uk/WRcat/index.php|access-date=2021-05-28|website=pacrowther.staff.shef.ac.uk}}</ref>
|<ref name=":0" />
|-
|[HC2007] 31
|160,000?
|
|
|[[볼프-레이에별|WO3]]
|12,886,000
|<ref>{{저널 인용|last1=Hadfield|first1=L. J.|last2=Crowther|first2=P. A.|date=October 2007|title=A survey of the Wolf-Rayet population of the barred, spiral galaxy NGC 1313|bibcode=2007MNRAS.381..418H|journal=Monthly Notices of the Royal Astronomical Society|language=en|volume=381|issue=1|pages=418–432|doi=10.1111/j.1365-2966.2007.12284.x|arxiv=0708.2039 |s2cid=3024190 |issn=0035-8711|doi-access=free}}</ref>
|-
|[[BAT99-53|BAT99-53 A]]
|158,000
|13
|224,000
|[[볼프-레이에별|WC4]]
|~160,000
|<ref>{{저널 인용|last1=Ramachandran|first1=V.|last2=Hamann|first2=W.-R.|last3=Hainich|first3=R.|last4=Oskinova|first4=L. M.|last5=Shenar|first5=T.|last6=Sander|first6=A. A. C.|last7=Todt|first7=H.|last8=Gallagher|first8=J. S.|date=2018-07-01|title=Stellar population of the superbubble N 206 in the LMC. II. Parameters of the OB and WR stars, and the total massive star feedback|bibcode=2018A&A...615A..40R|journal=Astronomy and Astrophysics|volume=615|pages=A40|doi=10.1051/0004-6361/201832816|arxiv=1802.07494|issn=0004-6361|doi-access=free}}</ref>
|-
|[[IC 1613]] DR1
|150,000
|20
|480,000
|[[볼프-레이에별|WO3]]
|~2,380,000
|<ref>{{저널 인용|bibcode=2013A&A...559A..72T|arxiv=1310.2849|title=On the nature of WO stars: A quantitative analysis of the WO3 star DR1 in IC 1613|journal=Astronomy & Astrophysics|volume=559|pages=A72|last1=Tramper|first1=F.|last2=Gräfener|first2=G.|last3=Hartoog|first3=O. E.|last4=Sana|first4=H.|last5=De Koter|first5=A.|last6=Vink|first6=J. S.|last7=Ellerbroek|first7=L. E.|last8=Langer|first8=N.|last9=Garcia|first9=M.|last10=Kaper|first10=L.|last11=De Mink|first11=S. E.|author11-link= Selma de Mink |year=2013|doi=10.1051/0004-6361/201322155|s2cid=216079684 }}</ref>
|-
|[[LH41-1042]]
|150,000
|8.4
|182,000
|[[볼프-레이에별|WO4]]
|~160,000
|<ref name="tramper">{{저널 인용|bibcode=2015A&A...581A.110T|arxiv=1507.00839|title=Massive stars on the verge of exploding: The properties of oxygen sequence Wolf-Rayet stars|journal=Astronomy & Astrophysics|volume=581|pages=A110|last1=Tramper|first1=F.|last2=Straal|first2=S. M.|last3=Sanyal|first3=D.|last4=Sana|first4=H.|last5=De Koter|first5=A.|last6=Gräfener|first6=G.|last7=Langer|first7=N.|last8=Vink|first8=J. S.|last9=De Mink|first9=S. E.|author9-link= Selma de Mink |last10=Kaper|first10=L.|year=2015|doi=10.1051/0004-6361/201425390|s2cid=56093231 }}</ref>
|-
|[[BAT99-2]]
|141,000
|13
|234,000
|[[볼프-레이에별|WN2]]
|~160,000
|<ref name=":2">{{저널 인용|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.|date=May 2014|title=The Wolf-Rayet stars in the Large Magellanic Cloud. A comprehensive analysis of the WN class|url=https://ui.adsabs.harvard.edu/abs/2014A&A...565A..27H/abstract|journal=Astronomy and Astrophysics|language=en|volume=565|pages=A27|doi=10.1051/0004-6361/201322696|issn=0004-6361|arxiv=1401.5474|bibcode=2014A&A...565A..27H |s2cid=55123954 }}</ref>
|-
|[[WR 2]]
|141,000
|16
|282,000
|[[볼프-레이에별|WN2]]
|7,830<ref name=":1" />
|
|-
|[[SMC AB8|AB8]]
|141,000
|19
|1,413,000
|[[볼프-레이에별|WO4]]
|197,000
|<ref name=tramper/>
|-
|[[BA 1-458]]
|140,000
|28.1
|776,000
|[[볼프-레이에별|WO4]]
|2,500,000
|<ref>{{저널 인용|last=Abbott|first=Jay Brian|date=2004|title=Quantitative spectroscopic studies of Wolf-Rayet stars in local group galaxies|url=https://ui.adsabs.harvard.edu/abs/2004PhDT.......161A/abstract|journal=Ph.D. Thesis|bibcode=2004PhDT.......161A |language=en}}</ref>
|-
|[[WR 9]] (WR)
|139,700
|9
|501,000
|[[볼프-레이에별|WC4]]
|14,900<ref name=":1" />
|
|-
|[[WR 30a]] (WR)
|129,500
|7.5-9.7
|195,000
|[[볼프-레이에별|WO4]]
|25,340
|<ref name=nugis>{{저널 인용|bibcode=2000A&A...360..227N|title=Mass-loss rates of Wolf-Rayet stars as a function of stellar parameters|journal=Astronomy and Astrophysics|volume=360|pages=227|last1=Nugis|first1=T.|last2=Lamers|first2=H. J. G. L. M.|year=2000}}</ref>
|-
|[[WR 38]]
|126,000
|10.4
|162,000
|[[볼프-레이에별|WC4]]
|
|<ref name=":0" />
|-
|[[WR 1]]
|112,200
|27
|759,000
|[[볼프-레이에별|WN4-s]]
|10,300<ref name=":1" />
|<ref name=":3">{{저널 인용|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.|date=2019-05-01|title=The Galactic WN stars revisited. Impact of Gaia distances on fundamental stellar parameters|url=http://adsabs.harvard.edu/abs/2019A%26A...625A..57H|journal=Astronomy and Astrophysics|volume=625|pages=A57|doi=10.1051/0004-6361/201834850|issn=0004-6361|arxiv=1904.04687|bibcode=2019A&A...625A..57H |s2cid=104292503 }}</ref>
|-
|[[WR 18]]
|112,200
|38
|1,288,000
|[[볼프-레이에별|WN4-s]]
|12,500<ref name=":1" />
|<ref name=":3" />
|-
|[[WR 46]]
|112,200
|14
|263,000
|[[볼프-레이에별|WN3pw]]
|13,000
|
|-
|[[WR 7]]
|112,000
|13
|214,000
|[[볼프-레이에별|WN4-s]]
|14,000
|<ref name=":3" />
|-
|[[WR 144]]
|112,000
|9.9
|159,000
|[[볼프-레이에별|WC4]]
|5,710<ref name=":1" />
|<ref name=":0" />
|-
|WR 52
|112,000
|8.5
|117,000
|[[볼프-레이에별|WC4]]
|5,710<ref name=":1" />
|<ref name=":0" />
|-
|[[AB7]]
|105,000
|23
|1,259,000
|[[볼프-레이에별|WN4]]
|197,000
|<ref name=shenar>{{저널 인용|bibcode=2016A&A...591A..22S|title=Wolf-Rayet stars in the Small Magellanic Cloud: II. Analysis of the binaries|volume=1604|pages=A22|arxiv=1604.01022|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.|year=2016|doi=10.1051/0004-6361/201527916|journal=Astronomy & Astrophysics|s2cid=119255408 }}</ref>
|-
|[[WR 143]] (WR)
|100,000
|8?
|89,100
|[[볼프-레이에별|WC4]]
|7,240
|{{출처|날짜=2021-05}}
|-
|[[큰개자리 EZ]]
|89,100
|23
|617,000
|[[볼프-레이에별|WN4-s]]
|5,900{{출처|날짜=2021-05}}
|<ref name="wn">{{저널 인용|arxiv=1904.04687|last1=Sota|first1=A.|title=The Galactic WN stars revisited. Impact of Gaia distances on fundamental stellar parameters|last2=Maíz Apellániz|first2=J.|last3=Morrell|first3=N. I.|last4=Barbá|first4=R. H.|last5=Walborn|first5=N. R.|last6=Gamen|first6=R. C.|last7=Arias|first7=J. I.|last8=Alfaro|first8=E. J.|last9=Oskinova|first9=L. M.|journal=Astronomy & Astrophysics|year=2019|volume=A57|page=625|doi=10.1051/0004-6361/201834850|bibcode=2019A&A...625A..57H|s2cid=104292503}}</ref>
|-
|[[WR 36]]
|89,100
|12
|200,000
|[[볼프-레이에별|WN5-s]]
|17,700<ref name=":1" />
|<ref name=":3" />
|-
|[[WR 111]]
|89,100
|13
|245,000
|[[볼프-레이에별|WC5]]
|5,320<ref name=":1" />
|<ref name=":0" />
|-
|[[WR 150]]
|89,100
|24.8
|724,000
|[[볼프-레이에별|WC5]]
|28,500<ref name=":1" />
|<ref name=":0" />
|-
|[[파리자리 세타]]
|83,000
|
|234,000
|[[볼프-레이에별|WC5]]
|7,500
|
|-
|[[살쾡이자리 원호]]의 항성들
|80,000
|
|
|
|12,000,000,000
|
|-
|[[WR 19|WR 19 A]]
|79,400
|
|400,000
|[[볼프-레이에별|WC5d]]
|14,000<ref name=":1" />
|<ref name="Galactic Wolf Rayet Catalogue">{{웹 인용|url=http://pacrowther.staff.shef.ac.uk/WRcat/ |title=Galactic Wolf Rayet Catalogue |author=Paul Crowther |author-link=Paul Crowther |access-date=2021-05-27 }}</ref><ref>{{저널 인용|last1=Lau|first1=Ryan M.|last2=Eldridge|first2=J. J.|last3=Hankins|first3=Matthew J.|last4=Lamberts|first4=Astrid|last5=Sakon|first5=Itsuki|last6=Williams|first6=Peredur M.|date=2020-07-01|title=Revisiting the Impact of Dust Production from Carbon-rich Wolf-Rayet Binaries|bibcode=2020ApJ...898...74L|journal=The Astrophysical Journal|volume=898|issue=1|pages=74|doi=10.3847/1538-4357/ab9cb5|arxiv=2006.08695|s2cid=219708543 |issn=0004-637X |doi-access=free }}</ref>
|-
|[[WR 44]]
|79,400
|18
|417,000
|[[볼프-레이에별|WN4-w]]
|19,800<ref name=":1" />
|<ref name=":3" />
|-
|[[WR 58]]
|79,000
|8.4
|89,100
|[[볼프-레이에별|WN4/WCE]]
|19,700<ref name=":1" />
|<ref name=":0" />
|-
|[[BAT99-37]]
|79,000
|19
|447,000
|[[볼프-레이에별|WN3o]]
|160,000
|<ref name=":2" />
|-
|[[WR 45]]
|79,000
|14.1
|282,000
|[[볼프-레이에별|WC6]]
|13,900<ref name=":1" />
|<ref name=":0" />
|-
|[[WR 86]]
|70,800
|
|
|[[볼프-레이에별|WC7]]
|
|{{출처|날짜=2021-05}}
|-
|[[WR 136]]
|70,800
|15
|260,000
|[[볼프-레이에별|WN6(h)-s]]
|6,290<ref name=":1" />
|
|-
|[[WR 75]]
|63,100
|18
|389,000
|[[볼프-레이에별|WN6-s]]
|10,800<ref name=":1" />
|<ref name=":3" />
|-
|[[WR 134]]
|63,100
|19
|400,000
|[[볼프-레이에별|WN6-s]]
|6,000
|
|-
|[[WR 60]]
|63,100
|23
|631,000
|[[볼프-레이에별|WC8]]
|11,500<ref name=":1" />
|<ref name=":0" />
|-
|[[WR 149]]
|63,100
|14
|269,000
|[[볼프-레이에별|WN5-s]]
|15,900<ref name=":1" />
|<ref name=":3" />
|-
|[[다섯쌍둥이 성단|WR102f]]
|60,000
|
|200,000
|[[볼프-레이에별|WC8]]
|26,000
|
|-
|}

== 같이 보기 ==
* [[질량이 큰 항성 목록]]
* [[광도 순 항성 목록]]
* [[질량이 작은 항성 목록]]
* [[유효온도가 낮은 항성 목록]]

== 각주 ==
{{각주}}

{{항성}}
{{포털 막대|천문학|우주 개발|우주 공간|태양계}}

[[분류:항성 목록]]