Hostname: page-component-cd9895bd7-p9bg8 Total loading time: 0 Render date: 2024-12-23T20:02:22.848Z Has data issue: false hasContentIssue false
  • English
  • Français

Emission Line Variability in the Be Star X-Ray Binaries 4U1258-61 and 4U2206+54

Published online by Cambridge University Press:  23 September 2016

Robin H.D. Corbet
Robin H.D. Corbet*
Affiliation:
Department of Astrophysics, University of Oxford, South Parks Rd., Oxford, 0X1 3RQ, U.K.

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Results of programs to monitor Ha emission line variability in two Be star X-ray binaries are presented. These systems provide a means of investigating the influence of a binary companion on the circumstellar envelope of a Be star.

Type
III. The Circumstellar Gas
Information
International Astronomical Union Colloquium , Volume 92: Physics of Be Stars , August 1987 , pp. 311 - 313
Copyright
Copyright © Cambridge University Press 1987

References

Corbet, R.H.D., Smale, A.P., Menzies, J.W., Branduardi-Raymont, G., Charles, P.A., Mason, K.O., & Booth, L. (1986). MNRAS, 221, 961.CrossRefGoogle Scholar
Marlborough, J.M., Snow, T.P., & Slettebak, A. (1978). Ap. J., 224, 157.CrossRefGoogle Scholar
Poeckert, R. (1982). In “Be stars”, IAU Symp. no. 98., eds. Jaschek, M. & Groth, H.-G., p.453. Google Scholar
Steiner, J.E., Ferrara, A., Garcia, M., Patterson, J., Schwartz, D.A., Warwick, R.S., Watson, M.G. & McClintock, J.E. (1984). Ap. J., 280, 688.Google Scholar