The outburst radial velocity curve of X-Ray Nova Scorpii 1994 (=GRO J1655--40)
We present a re-analysis 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 (K2, q) plane which, when combined with the publishe...
| 主要な著者: | , , |
|---|---|
| フォーマット: | Journal article |
| 出版事項: |
Oxford University Press
1999
|
| 要約: | We present a re-analysis 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 (K2, 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 |
|---|