Journal article
The outburst radial velocity curve of X-Ray Nova Scorpii 1994 (=GRO J1655--40)
- Abstract:
- 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
- Publication status:
- Published
- Peer review status:
- Peer reviewed
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(Preview, Version of record, pdf, 285.3KB, Terms of use)
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- Publisher copy:
- 10.1046/j.1365-8711.1999.02357.x
Authors
- Publisher:
- Oxford University Press
- Journal:
- Monthly Notices of the Royal Astronomical Society More from this journal
- Volume:
- 304
- Issue:
- 4
- Pages:
- 839-844
- Publication date:
- 1999-04-16
- Acceptance date:
- 1998-12-07
- DOI:
- EISSN:
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1365-2966
- ISSN:
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0035-8711
- Keywords:
- Pubs id:
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pubs:205436
- UUID:
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uuid:99a1cd3c-9b9e-4f8c-9f5c-44240a4dbb94
- Local pid:
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pubs:205436
- Source identifiers:
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205436
- Deposit date:
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2013-02-20
Terms of use
- Copyright holder:
- Royal Astronomical Society
- Copyright date:
- 1999
- Notes:
- © 1999 RAS. This is the publisher's version of the article. The final version is available online from Oxford University Press at: https://doi.org/10.1046/j.1365-8711.1999.02357.x
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