A0620-00

A0620-00 (V616 Monocerotis, V616 Mon) is a low-mass X-ray binary star and black-hole candidate in the constellation of Monoceros.[1][2]

Evidence from observation

One of the components of the A0620-00 binary system is known to be a dark, compact stellar object, with a mass between 6.3 and 6.9 times the mass of the Sun. The other component is observed to be a K-type star (approximately 0.5 solar masses).[3][4][5][6]

Significance

This binary system is located at a distance of approximately 3,000 light years, making the system the likely location of the nearest known black hole.[7]

See also

References

  1. ↑ 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.
  2. ↑ Thomas E. Harrison, Steve B. Howell, Paula Szkody, France A. Cordova; "The Nature of the Secondary Star in the Black Hole X-Ray Transient V616 Mon (=A0620-00)"; The Astronomical Journal, Volume 133, Issue 1, pp. 162-168. January 2007; arXiv:astro-ph/0609535 ; Bibcode: 2007AJ....133..162H ; doi:10.1086/509572
  3. ↑ University of Texas observatory Archived 1 April 2012 at the Wayback Machine. retrieved 19 September 2011
  4. ↑ Abstract- T.R.Marsh,E.L.Robinson,J.H.Woods absabs.harvard retrieved 24 July 2010
  5. ↑ T.R.Marsh,E.L.Robinson,J.H.Wood (1993) The Royal Astronomical Society (copyright) retrieved 19 September 2011
  6. ↑ Cantrell, Andrew G. (20 February 2010). "The Inclination of the Soft X-ray Transient A0620−00 and the Mass of Its Black Hole". The Astrophysical Journal. The American Astronomical Society. 720: 1127–1141.
  7. ↑ University of Texas observatory retrieved 21 March 2016
This article is issued from Wikipedia. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.