Astronomy:List of hottest stars
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Short description: 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
| Star name | Effective Temperature (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 87 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] | |
| LH41-1042 | 150,000 | 8.4 | 182,000 | WO4 | ~160,000 | ||
| 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 | [11] | |
| 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 | [12] | |
| WR 38 | 126,000 | 10.4 | 724,000[13] | WC4 | 19,700[13] | [3] | |
| WR 142a | 125,000 | 7.9 | 110,000 | WC8 | 5,900[13] | [14] | |
| BAT99-128 | 112,000 | 14 | 275,000 | WN3 | ~160,000 | [9] | |
| WR 1 | 112,000 | 27 | 759,000 | WN4-s | 10,300[1] | [15] | |
| WR 18 | 112,000 | 38 | 1,288,000 | WN4-s | 12,500[1] | [15] | |
| WR 46 | 112,000 | 14 | 263,000 | WN3pw | 13,000 | ||
| WR 7 | 112,000 | 13 | 214,000 | WN4-s | 14,000 | [15] | |
| 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 | [16] | |
| BAT99-24 | 100,000 | 17 | 347,000 | WN4b | ~160,000 | [9] | |
| WR 37 | 100,000 | 34 | 1,122,000 | WN4-s | 21,900[13] | ||
| NGC 6822-WR 12 | 100,000 | 36 | 1,288,000 | WN4 | ~1,631,000 | [11] | |
| Gamma Velorum (WR) | 90,000 | 9 | 204,000 | WC8 | 1,100 | A quadruple star system | [17] |
| BAT99-1 | 89,100 | 12 | 200,000 | WN3b | ~160,000 | [9] | |
| EZ CMa | 89,100 | 23 | 617,000 | WN4-s | A Wolf-Rayet star that may be an eccentric binary star system.[18] | [19] | |
| WR 36 | 89,100 | 12 | 200,000 | WN5-s | 17,700[1] | [15] | |
| 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] | |||
| WR 44 | 79,400 | 18 | 417,000 | WN4-w | 19,800[1] | [15] | |
| 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[20] | |
| WR 75 | 63,100 | 18 | 389,000 | WN6-s | 10,800[1] | [15] | |
| WR 134 | 63,100 | 19 | 400,000 | WN6-s | 6,000 | A Wolf-Rayet star that is very bright | [15] |
| WR 60 | 63,100 | 23 | 631,000 | WC8 | 11,500[1] | [3] | |
| WR 149 | 63,100 | 14 | 269,000 | WN5-s | 15,900[1] | [15] |
See also
- List of most massive stars
- List of most luminous stars
- List of least massive stars
- List of coolest stars
References
- ↑ 1.00 1.01 1.02 1.03 1.04 1.05 1.06 1.07 1.08 1.09 1.10 1.11 1.12 1.13 1.14 1.15 1.16 1.17 1.18 "Wolf-Rayet Star Catalogue". http://pacrowther.staff.shef.ac.uk/WRcat/index.php.
- ↑ Sander, A.; Hamann, W. -R.; Todt, H. (2012). "The Galactic WC stars". Astronomy & Astrophysics 540: A144. doi:10.1051/0004-6361/201117830. Bibcode: 2012A&A...540A.144S.
- ↑ 3.00 3.01 3.02 3.03 3.04 3.05 3.06 3.07 3.08 3.09 3.10 Sander, 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. doi:10.1051/0004-6361/201833712. ISSN 0004-6361. Bibcode: 2019A&A...621A..92S.
- ↑ 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" (in en). The Astrophysical Journal 715 (2): 1327–1337. doi:10.1088/0004-637X/715/2/1327. ISSN 0004-637X. Bibcode: 2010ApJ...715.1327S. https://ui.adsabs.harvard.edu/abs/2010ApJ...715.1327S/abstract.
- ↑ Massey, Philip (2014). "A modern search for Wolf–Rayet stars in the Magellanic Clouds: First results". The Astrophysical Journal 788 (1): 83. doi:10.1088/0004-637X/788/1/83. Bibcode: 2014ApJ...788...83M.
- ↑ 6.0 6.1 Cite error: Invalid
<ref>tag; no text was provided for refs namedtramper - ↑ Hadfield, L. J.; Crowther, P. A. (October 2007). "A survey of the Wolf-Rayet population of the barred, spiral galaxy NGC 1313" (in en). Monthly Notices of the Royal Astronomical Society 381 (1): 418–432. doi:10.1111/j.1365-2966.2007.12284.x. ISSN 0035-8711. Bibcode: 2007MNRAS.381..418H.
- ↑ 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. doi:10.1051/0004-6361/201832816. ISSN 0004-6361. Bibcode: 2018A&A...615A..40R.
- ↑ 9.00 9.01 9.02 9.03 9.04 9.05 9.06 9.07 9.08 9.09 9.10 Hainich, R.; Rühling, U.; Todt, H.; Oskinova, L. M.; Liermann, A.; Gräfener, G.; Foellmi, C.; Schnurr, O. et al. (May 2014). "The Wolf-Rayet stars in the Large Magellanic Cloud. A comprehensive analysis of the WN class" (in en). Astronomy and Astrophysics 565: A27. doi:10.1051/0004-6361/201322696. ISSN 0004-6361. Bibcode: 2014A&A...565A..27H. https://ui.adsabs.harvard.edu/abs/2014A&A...565A..27H/abstract.
- ↑ Kingsburgh, Robin L.; Barlow, M. J. (May 1995). "DR 1: a WO3 star in IC 1613 and its surrounding nebula, S3." (in en). Astronomy and Astrophysics 295: 171–182. ISSN 0004-6361. Bibcode: 1995A&A...295..171K. https://ui.adsabs.harvard.edu/abs/1995A&A...295..171K/abstract.
- ↑ 11.0 11.1 Abbott, Jay Brian (2004). "Quantitative spectroscopic studies of Wolf-Rayet stars in local group galaxies" (in en). Ph.D. Thesis. Bibcode: 2004PhDT.......161A. https://ui.adsabs.harvard.edu/abs/2004PhDT.......161A/abstract.
- ↑ 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.
- ↑ 13.0 13.1 13.2 13.3 Rate, 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. doi:10.1093/mnras/stz3614. ISSN 0035-8711. Bibcode: 2020MNRAS.493.1512R.
- ↑ 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. doi:10.1051/0004-6361:20021373. ISSN 0004-6361. Bibcode: 2002A&A...396..533P. https://ui.adsabs.harvard.edu/abs/2002A&A...396..533P.
- ↑ 15.0 15.1 15.2 15.3 15.4 15.5 15.6 15.7 Hamann, W.-R.; Gräfener, G.; Liermann, A.; Hainich, R.; Sander, A. A. C.; Shenar, T.; Ramachandran, V.; Todt, H. et al. (2019-05-01). "The Galactic WN stars revisited. Impact of Gaia distances on fundamental stellar parameters". Astronomy and Astrophysics 625: A57. doi:10.1051/0004-6361/201834850. ISSN 0004-6361. Bibcode: 2019A&A...625A..57H. http://adsabs.harvard.edu/abs/2019A%26A...625A..57H.
- ↑ Shenar, T.; Hainich, R.; Todt, H.; Sander, A.; Hamann, W.-R.; Moffat, A. F. J.; Eldridge, J. J.; Pablo, H. et al. (2016). "Wolf-Rayet stars in the Small Magellanic Cloud: II. Analysis of the binaries". Astronomy & Astrophysics 1604: A22. doi:10.1051/0004-6361/201527916. Bibcode: 2016A&A...591A..22S.
- ↑ 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. doi:10.1093/mnras/stae145. ISSN 0035-8711. Bibcode: 2024MNRAS.528.2026C.
- ↑ Koenigsberger, Gloria; Schmutz, Werner (2020-05-12), "The nature of the companion in the Wolf-Rayet system EZ Canis Majoris", Astronomy & Astrophysics 639: A18, doi:10.1051/0004-6361/201937305, Bibcode: 2020A&A...639A..18K, http://arxiv.org/abs/2005.06028, 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. et al. (2019). "The Galactic WN stars revisited. Impact of Gaia distances on fundamental stellar parameters". Astronomy & Astrophysics A57: 625. doi:10.1051/0004-6361/201834850. Bibcode: 2019A&A...625A..57H.
- ↑ 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. doi:10.1093/mnras/stv1423. ISSN 0035-8711.
