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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.〔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.〕〔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; ; ; 〕 ==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 nine and thirteen times the mass of the Sun. The other component is observed to be a K-type star (approximately 0.5 solar masses).〔(University of Texas observatory ) retrieved 19/09/2011〕〔Abstract- T.R.Marsh,E.L.Robinson,J.H.Woods (absabs.harvard ) retrieved 24/7/2010〕〔T.R.Marsh,E.L.Robinson,J.H.Wood (1993) ( The Royal Astronomical Society (copyright) ) retrieved 19/09/2011〕
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