A0620-00是位于麒麟座的恒星质量黑洞候选者[5]。它位于一个双星系统中,其中一颗质量较大,而另一颗质量比较小,大质量的恒星变成黑洞。它的质量目前估计是太阳质量的6
.6倍[2]。
参考资料
- ^ 1.00 1.01 1.02 1.03 1.04 1.05 1.06 1.07 1.08 1.09 [ 1A 0620-00]. SIMBAD. 斯特拉斯堡天文資料中心. [26 August 2017].
- ^ 2.0 2.1 2.2 2.3 2.4 Cantrell, Andrew G.; Bailyn, Charles D.; Orosz, Jerome A.; McClintock, Jeffrey E.; Remillard, Ronald A.; Froning, Cynthia S.; Neilsen, Joseph; Gelino, Dawn M.; Gou, Lijun. The Inclination of the Soft X-Ray Transient A0620-00 and the Mass of its Black Hole. The Astrophysical Journal. 2010, 710 (2): 1127–1141. Bibcode:2010ApJ...710.1127C. arXiv:1001.0261
. doi:10.1088/0004-637X/710/2/1127.
- ^ Samus, N. N.; Durlevich, O. V.; et al. VizieR Online Data Catalog: General Catalogue of Variable Stars (Samus+ 2007-2013). VizieR On-line Data Catalog: B/gcvs. Originally published in: 2009yCat....102025S. 2009, 1. Bibcode:2009yCat....102025S.
- ^ 4.0 4.1 4.2 4.3 McClintock, J. E.; Remillard, R. A. The black hole binary A0620-00. Astrophysical Journal. 1986, 308: 110–122. Bibcode:1986ApJ...308..110M. doi:10.1086/164482.
- ^ Gelino, Dawn M., et al. "A Multiwavelength, Multiepoch Study of the Soft X-Ray Transient Prototype, V616 Monocerotis (A0620-00)". The Astronomical Journal, Volume 122, Issue 5, pp. 2668-2678, November 2001.