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Infrared spectroscopy of V616 Mon (=A0620--00): the accretion disc contamination

1999/02/22 by T. Shahbaz, Shahbaz, T., R. M. Bandyopadhyay +3
Engineering · Physics and Astronomy · #Astrophysical Phenomena and Observations #Astrophysics (astro-ph) #FOS: Physical sciences #Mechanics and Biomechanics Studies #astro-ph

paper · pdf · doi:10.48550/arxiv.astro-ph/9902312

7 pages, 2 figures, Accepted by A&A

arxiv created 1999/02/22 · openalex publication_date 1999/02/22 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28

Abstract

We have obtained for the first time K-band infrared spectra of the soft X-ray transient V616 Mon (=A0620--00). We determine the 2-sigma upper limit to the fraction of light arising from the accretion disc to be 27 percent. The effect this has on the binary inclination, determined from modelling the infrared ellipsoidal variations is to increase it by less than 7 degrees and decrease the mass of the black hole by less than 3.6 Msun.

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