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Astron. Astrophys. 346, 82-86 (1999)


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

T. Shahbaz, R.M. Bandyopadhyay and P.A. Charles

Department of Astrophysics, Oxford University, Keble Road, Oxford OX1 3RH, UK

Received 16 July 1998 / Accepted 22 February 1999

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-[FORMULA] 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 [FORMULA].

Key words: stars: binaries: general – stars: fundamental parameters – stars: individual: V616 Mon (A0620 – 00) – X-rays: stars

Send offprint requests to: T. Shahbaz (tsh@astro.ox.ac.uk)

© European Southern Observatory (ESO) 1999

Online publication: May 6, 1999

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