Appearance move to sidebar hide From Wikipedia, the free encyclopedia Nebula ejecta from the star WR 102 List of the hottest known stars
This is a list of hottest stars so far discovered (excluding degenerate stars), arranged by decreasing temperature. The stars with temperatures higher than 60,000 K are included.
List
[edit]
This list is incomplete; you can help by adding missing items. (May 2015)
Star name
EffectiveTemperature(K)
Mass(M☉)
Luminosity(L☉)
Spectral type
Distance(light-years)
Description
Ref.
WR 102
200,000
16.1
380,000
WO2
8,610[1]
[2][3]
WR 142
200,000
28.6
912,000
WO2
5,400
Very young oxygen type WO star on the Berkeley star cluster.[4]
[3]
LMC195-1
200,000
257,000
WO2
~160,000
[5]
BAT99-123
170,000
7.7
158,000
WO3
~160,000
[6]
WR 93b
160,000
8.1
110,000
WO3
7,470[1]
A WO star with stellar wind speeds of 5750 km/s making it the record holder.
[3]
[HC2007] 31
160,000?
WO3
12,886,000
[7]
BAT99-53 A
158,000
13
224,000
WC4
~160,000
[8]
BAT99-7
158,000
25
692,000
WN4b
~160,000
[9]
IC 1613 DR1
150,000
20
480,000
WO3
~2,380,000
A Wolf-Rayet star located in the dwarf galaxy IC 1613. It is surrounded by a nebula.[10]
[11]
LH41-1042
150,000
8.4
182,000
WO4
~160,000
[6]
BAT99-2
141,000
13
234,000
WN2
~160,000
[9]
BAT99-94
141,000
24
631,000
WN3
~160,000
[9]
WR 2
141,000
16
282,000
WN2
7,830[1]
AB8
141,000
19
1,413,000
WO4
~197,000
[6]
BA 1-458
140,000
28.1
776,000
WO4
2,500,000
[12]
WR 9 (WR)
139,700
9
501,000
WC4
14,900[1]
WR 30a (WR)
129,500
7.5-9.7
195,000
WO4
25,340
[13]
WR 38
126,000
10.4
724,000[14]
WC4
19,700[14]
[3]
WR 142a
125,000
7.9
110,000
WC8
5,900[14]
[15]
BAT99-128
112,000
14
275,000
WN3
~160,000
[9]
WR 1
112,000
27
759,000
WN4-s
10,300[1]
[16]
WR 18
112,000
38
1,288,000
WN4-s
12,500[1]
[16]
WR 46
112,000
14
263,000
WN3pw
13,000
WR 7
112,000
13
214,000
WN4-s
14,000
[16]
WR 144
112,000
9.9
159,000
WC4
5,710[1]
[3]
WR 52
112,000
8.5
117,000
WC4
5,710[1]
[3]
AB7
105,000
23
1,259,000
WN4
~197,000
[17]
BAT99-24
100,000
17
347,000
WN4b
~160,000
[9]
WR 37
100,000
34
1,122,000
WN4-s
21,900[14]
NGC 6822-WR 12
100,000
36
1,288,000
WN4
~1,631,000
[12]
Gamma Velorum (WR)
90,000
9
204,000
WC8
1,100
A quadruple star system
[18]
BAT99-1
89,100
12
200,000
WN3b
~160,000
[9]
EZ CMa
89,100
23
617,000
WN4-s
5,900[citation needed]
A Wolf-Rayet star that may be an eccentric binary star system.[19]
[20]
WR 36
89,100
12
200,000
WN5-s
17,700[1]
[16]
WR 111
89,100
13
245,000
WC5
5,320[1]
[3]
WR 150
89,100
24.8
724,000
WC5
28,500[1]
[3]
BAT99-3
79,400
16
324,000
WN4b
~160,000
[9]
WR 19 A
79,400
400,000
WC5d
14,000[1]
[21][22]
WR 44
79,400
18
417,000
WN4-w
19,800[1]
[16]
WR 58
79,400
8.4
89,100
WN4/WCE
19,700[1]
[3]
BAT99-37
79,400
19
447,000
WN3o
160,000
[9]
WR 45
79,400
14.1
282,000
WC6
13,900[1]
[3]
BAT99-26
70,800
18
417,000
WN4b
~160,000
[9]
BAT99-35
70,800
24
398,000
WN3(h)
~160,000
[9]
BAT99-86
70,800
12
427,000
WN3(h)
~160,000
[9]
WR 136
70,800
15
260,000
WN6(h)-s
6,290[1]
Fast stellar winds created the Crescent nebula[23]
WR 75
63,100
18
389,000
WN6-s
10,800[1]
[16]
WR 134
63,100
19
400,000
WN6-s
6,000
A Wolf-Rayet star that is very bright
[16]
WR 60
63,100
23
631,000
WC8
11,500[1]
[3]
WR 149
63,100
14
269,000
WN5-s
15,900[1]
[16]
See also
[edit]
List of most massive stars
List of most luminous stars
List of least massive stars
List of coolest stars
References
[edit]
^ abcdefghijklmnopqrs"Wolf-Rayet Star Catalogue". pacrowther.staff.shef.ac.uk. Retrieved 2021-05-28.
^Sander, A.; Hamann, W. -R.; Todt, H. (2012). "The Galactic WC stars". Astronomy & Astrophysics. 540: A144. arXiv:1201.6354. Bibcode:2012A&A...540A.144S. doi:10.1051/0004-6361/201117830. S2CID 119182468.
^ abcdefghijkSander, A. A. C.; Hamann, W.-R.; Todt, H.; Hainich, R.; Shenar, T.; Ramachandran, V.; Oskinova, L. M. (2019-01-01). "The Galactic WC and WO stars. The impact of revised distances from Gaia DR2 and their role as massive black hole progenitors". Astronomy and Astrophysics. 621: A92. arXiv:1807.04293. Bibcode:2019A&A...621A..92S. doi:10.1051/0004-6361/201833712. ISSN 0004-6361.
^Sokal, Kimberly R.; Skinner, Stephen L.; Zhekov, Svetozar A.; Güdel, Manuel; Schmutz, Werner (June 2010). "Chandra Detects the Rare Oxygen-type Wolf-Rayet Star WR 142 and OB Stars in Berkeley 87". The Astrophysical Journal. 715 (2): 1327–1337. arXiv:1004.0462. Bibcode:2010ApJ...715.1327S. doi:10.1088/0004-637X/715/2/1327. ISSN 0004-637X.
^Massey, Philip (2014). "A modern search for Wolf–Rayet stars in the Magellanic Clouds: First results". The Astrophysical Journal. 788 (1): 83. arXiv:1404.7441. Bibcode:2014ApJ...788...83M. doi:10.1088/0004-637X/788/1/83. S2CID 119177379.
^ abcTramper, F.; Straal, S. M.; Sanyal, D.; Sana, H.; De Koter, A.; Gräfener, G.; Langer, N.; Vink, J. S.; De Mink, S. E.; Kaper, L. (2015). "Massive stars on the verge of exploding: The properties of oxygen sequence Wolf-Rayet stars". Astronomy & Astrophysics. 581: A110. arXiv:1507.00839. Bibcode:2015A&A...581A.110T. doi:10.1051/0004-6361/201425390. S2CID 56093231.
^Hadfield, L. J.; Crowther, P. A. (October 2007). "A survey of the Wolf-Rayet population of the barred, spiral galaxy NGC 1313". Monthly Notices of the Royal Astronomical Society. 381 (1): 418–432. arXiv:0708.2039. Bibcode:2007MNRAS.381..418H. doi:10.1111/j.1365-2966.2007.12284.x. ISSN 0035-8711. S2CID 3024190.
^Ramachandran, V.; Hamann, W.-R.; Hainich, R.; Oskinova, L. M.; Shenar, T.; Sander, A. A. C.; Todt, H.; Gallagher, J. S. (2018-07-01). "Stellar population of the superbubble N 206 in the LMC. II. Parameters of the OB and WR stars, and the total massive star feedback". Astronomy and Astrophysics. 615: A40. arXiv:1802.07494. Bibcode:2018A&A...615A..40R. doi:10.1051/0004-6361/201832816. ISSN 0004-6361.
^ abcdefghijkHainich, R.; Rühling, U.; Todt, H.; Oskinova, L. M.; Liermann, A.; Gräfener, G.; Foellmi, C.; Schnurr, O.; Hamann, W.-R. (May 2014). "The Wolf-Rayet stars in the Large Magellanic Cloud. A comprehensive analysis of the WN class". Astronomy and Astrophysics. 565: A27. arXiv:1401.5474. Bibcode:2014A&A...565A..27H. doi:10.1051/0004-6361/201322696. ISSN 0004-6361. S2CID 55123954.
^Kingsburgh, Robin L.; Barlow, M. J. (May 1995). "DR 1: a WO3 star in IC 1613 and its surrounding nebula, S3". Astronomy and Astrophysics. 295: 171–182. Bibcode:1995A&A...295..171K. ISSN 0004-6361.
^Tramper, F.; Gräfener, G.; Hartoog, O. E.; Sana, H.; De Koter, A.; Vink, J. S.; Ellerbroek, L. E.; Langer, N.; Garcia, M.; Kaper, L.; De Mink, S. E. (2013). "On the nature of WO stars: A quantitative analysis of the WO3 star DR1 in IC 1613". Astronomy & Astrophysics. 559: A72. arXiv:1310.2849. Bibcode:2013A&A...559A..72T. doi:10.1051/0004-6361/201322155. S2CID 216079684.
^ abAbbott, Jay Brian (2004). "Quantitative spectroscopic studies of Wolf-Rayet stars in local group galaxies". Ph.D. Thesis. Bibcode:2004PhDT.......161A.
^Nugis, T.; Lamers, H. J. G. L. M. (2000). "Mass-loss rates of Wolf-Rayet stars as a function of stellar parameters". Astronomy and Astrophysics. 360: 227. Bibcode:2000A&A...360..227N.
^ abcdRate, Gemma; Crowther, Paul A. (2020-03-01). "Unlocking Galactic Wolf-Rayet stars with Gaia DR2 - I. Distances and absolute magnitudes". Monthly Notices of the Royal Astronomical Society. 493 (1): 1512–1529. arXiv:1912.10125. Bibcode:2020MNRAS.493.1512R. doi:10.1093/mnras/stz3614. ISSN 0035-8711.
^Pasquali, A.; Comerón, F.; Gredel, R.; Torra, J.; Figueras, F. (2002-12-01). "A new Wolf-Rayet star in Cygnus". Astronomy and Astrophysics. 396 (2): 533–538. arXiv:astro-ph/0210179. Bibcode:2002A&A...396..533P. doi:10.1051/0004-6361:20021373. ISSN 0004-6361.
^ abcdefghHamann, W.-R.; Gräfener, G.; Liermann, A.; Hainich, R.; Sander, A. A. C.; Shenar, T.; Ramachandran, V.; Todt, H.; Oskinova, L. M. (2019-05-01). "The Galactic WN stars revisited. Impact of Gaia distances on fundamental stellar parameters". Astronomy and Astrophysics. 625: A57. arXiv:1904.04687. Bibcode:2019A&A...625A..57H. doi:10.1051/0004-6361/201834850. ISSN 0004-6361. S2CID 104292503.
^Shenar, T.; Hainich, R.; Todt, H.; Sander, A.; Hamann, W.-R.; Moffat, A. F. J.; Eldridge, J. J.; Pablo, H.; Oskinova, L. M.; Richardson, N. D. (2016). "Wolf-Rayet stars in the Small Magellanic Cloud: II. Analysis of the binaries". Astronomy & Astrophysics. 1604: A22. arXiv:1604.01022. Bibcode:2016A&A...591A..22S. doi:10.1051/0004-6361/201527916. S2CID 119255408.
^Crowther, Paul A.; Barlow, M. J.; Royer, P.; Hillier, D. J.; Bestenlehner, J. M.; Morris, P. W.; Wesson, R. (2024-02-01). "Oxygen abundance of γ Vel from [O III] 88 μm Herschel/PACS spectroscopy". Monthly Notices of the Royal Astronomical Society. 528 (2): 2026–2039. arXiv:2310.15170. Bibcode:2024MNRAS.528.2026C. doi:10.1093/mnras/stae145. ISSN 0035-8711.
^Koenigsberger, Gloria; Schmutz, Werner (2020-05-12), "The nature of the companion in the Wolf-Rayet system EZ Canis Majoris", Astronomy & Astrophysics, 639: A18, arXiv:2005.06028, Bibcode:2020A&A...639A..18K, doi:10.1051/0004-6361/201937305, retrieved 2025-06-08
^Sota, A.; Maíz Apellániz, J.; Morrell, N. I.; Barbá, R. H.; Walborn, N. R.; Gamen, R. C.; Arias, J. I.; Alfaro, E. J.; Oskinova, L. M. (2019). "The Galactic WN stars revisited. Impact of Gaia distances on fundamental stellar parameters". Astronomy & Astrophysics. A57: 625. arXiv:1904.04687. Bibcode:2019A&A...625A..57H. doi:10.1051/0004-6361/201834850. S2CID 104292503.
^Paul Crowther. "Galactic Wolf Rayet Catalogue". Retrieved 2021-05-27.
^Lau, Ryan M.; Eldridge, J. J.; Hankins, Matthew J.; Lamberts, Astrid; Sakon, Itsuki; Williams, Peredur M. (2020-07-01). "Revisiting the Impact of Dust Production from Carbon-rich Wolf-Rayet Binaries". The Astrophysical Journal. 898 (1): 74. arXiv:2006.08695. Bibcode:2020ApJ...898...74L. doi:10.3847/1538-4357/ab9cb5. ISSN 0004-637X. S2CID 219708543.
^Reyes-Pérez, J.; Morisset, C.; Peña, M.; Mesa-Delgado, A. (2015-09-11). "A consistent spectral model of WR 136 and its associated bubble NGC 6888". Monthly Notices of the Royal Astronomical Society. 452 (2): 1764–1778. arXiv:1507.00051. doi:10.1093/mnras/stv1423. ISSN 0035-8711.
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