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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
Abstract
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