Tham khảo WR

Tham khảo WR_102ka

1 2 3 4 5 6 7 Skrutskie, M. F.; Cutri, R. M.; Stiening, R.; Weinberg, M. D.; Schneider, S.; Carpenter, J. M.; Beichman, C.; Capps, R.; Chester, T.; Elias, J.; Huchra, J.; Liebert, J.; Lonsdale, C.; Monet, D. G.; Price, S.; Seitzer, P.; Jarrett, T.; Kirkpatrick, J. D.; Gizis, J. E.; Howard, E.; Evans, T.; Fowler, J.; Fullmer, L.; Hurt, R.; Light, R.; Kopan, E. L.; Marsh, K. A.; McCallon, H. L.; Tam, R.; Van Dyk, S. (2006). “The Two Micron All Sky Survey (2MASS)”. The Astronomical Journal. 131 (2): 1163. Bibcode:2006AJ....131.1163S. doi:10.1086/498708.
1 2 3 4 5 6 7 8 Barniske, A.; Oskinova, L. M.; Hamann, W. -R. (2008). “Two extremely luminous WN stars in the Galactic center with circumstellar emission from dust and gas”. Astronomy and Astrophysics. 486 (3): 971. arXiv:0807.2476. Bibcode:2008A&A...486..971B. doi:10.1051/0004-6361:200809568.
↑ Oskinova, L. M.; Steinke, M.; Hamann, W. - R.; Sander, A.; Todt, H.; Liermann, A. (2013). “One of the most massive stars in the Galaxy may have formed in isolation”. Monthly Notices of the Royal Astronomical Society. 436 (4): 3357. arXiv:1309.7651. Bibcode:2013MNRAS.436.3357O. doi:10.1093/mnras/stt1817.
↑ Wolf-Rainer Hamann; Andreas Barniske; Adriane Liermann; Oskinova; Diana Pasemann; Ute Ruehling (2011). “The most luminous stars in the Galaxy and the Magellanic Clouds”. Société Royale des Sciences de Liège. 80: 98. arXiv:1012.1875v1. Bibcode:2011BSRSL..80...98H.
↑ Felli, M.; Testi, L.; Schuller, F.; Omont, A. (2002). “Young massive stars in the ISOGAL survey. II. The catalogue of bright YSO candidates”. Astronomy and Astrophysics. 392 (3): 971–990. arXiv:astro-ph/9905296. Bibcode:2002A&A...392..971F. doi:10.1051/0004-6361:20020973.
↑ Homeier, N. L.; Blum, R. D.; Pasquali, A.; Conti, P. S.; Damineli, A. (2003). “Results from a near infrared search for emission-line stars in the Inner Galaxy: Spectra of new Wolf-Rayet stars”. Astronomy & Astrophysics. 408: 153–159. arXiv:astro-ph/0306578. Bibcode:2003A&A...408..153H. doi:10.1051/0004-6361:20030989.
↑ Clark, J. S.; Larionov, V. M.; Arkharov, A. (2005). “On the population of galactic Luminous Blue Variables” (PDF). Astronomy & Astrophysics. 435: 239–246. Bibcode:2005A&A...435..239C. doi:10.1051/0004-6361:20042563.

Tài liệu tham khảo

WikiPedia: WR_102ka //arxiv.org/abs/0807.2476 //arxiv.org/abs/1012.1875v1 //arxiv.org/abs/1309.7651 //arxiv.org/abs/astro-ph/0306578 //arxiv.org/abs/astro-ph/9905296 //doi.org/10.1051%2F0004-6361:20020973 //doi.org/10.1051%2F0004-6361:20030989 //doi.org/10.1051%2F0004-6361:20042563 //doi.org/10.1051%2F0004-6361:200809568 //doi.org/10.1086%2F498708