The outburst radial velocity curve of X-Ray Nova Scorpii 1994 (=GRO J1655--40)

Details The outburst radial velocity curve of X-Ray Nova Scorpii 1994 (=GRO J1655--40) The outburst radial velocity curve of X-Ray Nova Scorpii 1994 (=GRO J1655--40)

1998-11-30

arxiv.org/abs/astro-ph/9811474v1

Astronomy and Astrophysics

Astrophysics

Accepted for MNRAS, 4 pages Latex, 4 figures

Scientific paper

We present a reanalysis of the outburst radial velocity data for X-Ray Nova Scorpii 1994. Using a model based on X-ray heating of the secondary star we suggest a more realistic treatment of the radial velocity data. Solutions are obtained in the (K_2,q) plane which, when combined with the published value for the binary mass ratio and inclination, constrain the mass of the black hole to within the region 4.1

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