Anexo:Estrellas más calientes
Esta es una lista de las estrellas más calientes descubiertas hasta ahora (excluidas las estrellas compactas), dispuestas por disminución de temperatura incluyendo sólo hasta las que tienen temperaturas superiores a los 60.000 K.
Listado[editar]
| Nombre | Temperatura (K) |
Masa (M☉) | Luminosidad (LSol) | Tipo espectral | Distancia (Año luz) | Ref. |
|---|---|---|---|---|---|---|
| WR 102 | 210,000 | 19 | 282,000 | WO2 | 9,800 | [1] |
| WR 142 | 200,000 | 20 | 245,000 | WO2 | 4,000 | [2] |
| LMC195-1 | 200,000 | WO2 | 160,000 | [3] | ||
| BAT 99-123 | 170,000 | 17 | 160,000 | WO3 | [4] | |
| WR 93b | 160,000 | 17 | 200,000 | WO3 | [4] | |
| IC 1613 DR1 | 150,000 | 20 | 480,000 | WO3 | [5] | |
| LH41 1042 | 150,000 | 17 | 180,000 | WO4 | [4] | |
| Sk188 | 150,000 | WO4 | [4] | |||
| WR 2 | 141,000 | WN2 | ||||
| AB8 | 141,000 | 19 | 1,400,000 | WO4 | 197,000 | |
| WR 30a | 129,500 | WO4 | [6] | |||
| WR 143 | 117,000 | WC4 | ||||
| WR 46 | 112,000 | 25 | 630,000 | WN3 | 13,000 | |
| HD 56925 | 112,000 | 16 | 280,000 | WN4-s | 14,000 | |
| AB7 | 105,000 | 23 | 1,259,000 | WN4 | 197,000 | [7] |
| AG Pegasi | 100,000 | 0.6 | 3,700 | WN6 | 3,100 | |
| EZ CMa | 85,000 | 20 | 380,000 | WN4 | 5,900 | |
| Theta Muscae | 83,000 | WC5 | 7,500 | |||
| The stars of Lynx Arc | 80,000 | 12,000,000,000 | ||||
| WR 45 | 78,000 | WC6 | ||||
| WR 86 | 71,000 | WC7 | ||||
| WR 136 | 70,800 | 15 | 260,000 | WN6(h)-s | 2,400 | |
| WR 19 | 70,000 | WN4 | [8] | |||
| WR 1 | 70,000 | WN4b | [8] | |||
| WR 134 | 63,100 | 19 | 400,000 | WN6-s | 6,000 | |
| WR 149 | 60,000 | WN5 | ||||
| WR102f | 60,000 | 200,000 | WC8 | 26,000 |
Véase también[editar]
Referencias[editar]
- ↑ Sander, A.; Hamann, W. -R.; Todt, H. (2012). «The Galactic WC stars». Astronomy & Astrophysics 540: A144. Bibcode:2012A&A...540A.144S. arXiv:1201.6354. doi:10.1051/0004-6361/201117830.
- ↑ Sokal, Kimberly R.; Skinner, Stephen L.; Zhekov, Svetozar A.; Güdel, Manuel; Schmutz, Werner (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. Bibcode:2010ApJ...715.1327S. arXiv:1004.0462. doi:10.1088/0004-637X/715/2/1327.
- ↑ Massey, Philip (2014). «A modern search for Wolf–Rayet stars in the Magellanic Clouds: First results». The Astrophysical Journal 788 (1): 83. Bibcode:2014ApJ...788...83M. doi:10.1088/0004-637X/788/1/83.
- ↑ a b c d Tramper, 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. Bibcode:2015A&A...581A.110T. arXiv:1507.00839. doi:10.1051/0004-6361/201425390.
- ↑ 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. Bibcode:2013A&A...559A..72T. arXiv:1310.2849. doi:10.1051/0004-6361/201322155.
- ↑ 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.
- ↑ 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. Bibcode:2016A&A...591A..22S. arXiv:1604.01022. doi:10.1051/0004-6361/201527916.
- ↑ a b Galactic Wolf Rayet Catalogue