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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

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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

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