Hostname: page-component-586b7cd67f-dsjbd Total loading time: 0 Render date: 2024-11-30T04:32:44.370Z Has data issue: false hasContentIssue false
  • English
  • Français

Ionization effects in stellar winds of massive X-ray binaries

Published online by Cambridge University Press:  12 April 2016

G. Hammerschlag-Hensberge
G. Hammerschlag-Hensberge*
Affiliation:
Astronomical Institute, University of Amsterdam

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.

High resolution ultraviolet spectroscopy of the early-type X-ray binary Vela X-l/HD 77581 provides a unique example to study the ionization structure of the stellar wind which varies under influence of the X-ray source. New results for other early-type X-ray binaries will be presented and compared with the Vela X-1 model. These results show that the observed variations strongly depend on the intensity of the X-ray source and on the density structure of the stellar wind.

Type
Session VIII - Effects of Mass Loss on the Evolution of Binary Stars
Information
International Astronomical Union Colloquium , Volume 59: Effects of Mass Loss on Stellar Evolution , 1981 , pp. 457 - 460
Copyright
Copyright © Reidel 1981

References

Dupree, A.K. et al.: 1980, Astrophys.J. 238, 969.CrossRefGoogle Scholar
Hatchett, S.P., and McCray, R.A.: 1977, Astrophys.J. 211, 552.CrossRefGoogle Scholar
McCray, R.A.: 1975, in Proc of the Calgary Conference on X-rays in Space, Calgary, pp.547.Google Scholar
Treves, A. et al.: 1980, Astrophys.J., in press.Google Scholar