1365-2966/asset/olbannerleft.gif?v=1&s=87f89c955da459679648fd327771ae82f16e5b8e)
1365-2966/asset/olbannerright.gif?v=1&s=08ebd3f71adfe4db0c1f9f65790c139e62520103)
Clumped stellar winds in supergiant high-mass X-ray binaries: X-ray variability and photoionization
Article first published online: 5 MAR 2012
DOI: 10.1111/j.1365-2966.2012.20507.x
© 2012 The Authors Monthly Notices of the Royal Astronomical Society © 2012 RAS
Issue
Monthly Notices of the Royal Astronomical Society
Volume 421, Issue 4, pages 2820–2831, April 2012
Additional Information
How to Cite
Oskinova, L. M., Feldmeier, A. and Kretschmar, P. (2012), Clumped stellar winds in supergiant high-mass X-ray binaries: X-ray variability and photoionization. Monthly Notices of the Royal Astronomical Society, 421: 2820–2831. doi: 10.1111/j.1365-2966.2012.20507.x
Publication History
- Issue published online: 10 APR 2012
- Article first published online: 5 MAR 2012
- Accepted 2012 January 5. Received 2012 January 5; in original form 2011 July 23
- Abstract
- Article
- References
- Supporting Information
- Cited By
Light curves. Synthetic X-ray light curves for Bondi-Hoyle accretion of a non-stationary stellar wind on to a NS with mX = 1.4 M⊙ for radii in the range 1.5R* to 30R*. The SG donor parameters are given in Table 1. The orbital separation a forms part of the filename. For example, xlc-a02.0.dat is an ASCII file that contains two columns: time and X-ray luminosity. The data in this file are for the orbital separation a = 2.0R*.
| Filename | Format | Size | Description |
|---|---|---|---|
| MNR_20507_sm_lightcurves.tar | 90K | Supporting info item |
Please note: Wiley-Blackwell is not responsible for the content or functionality of any supporting information supplied by the authors. Any queries (other than missing content) should be directed to the corresponding author for the article.