Hostname: page-component-cd9895bd7-dk4vv Total loading time: 0 Render date: 2024-12-26T19:42:39.560Z Has data issue: false hasContentIssue false
  • English
  • Français

The Structure of Colliding Stellar Winds

Published online by Cambridge University Press:  03 August 2017

A. Pollock ,
J. Blondin  and
I. Stevens
A. Pollock
Affiliation:
(1) EXOSAT Observatory, ESA/ESTEC, Noordwijk, Holland
J. Blondin
Affiliation:
(2) Astronomy Dept, University of Virginia, Charlottesville, VA 22903
I. Stevens
Affiliation:
(3) Code 665, NASA/GSFC, Greenbelt, Maryland, MD 20771

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.

We report on progress in the theoretical modelling of colliding winds in WR binary systems, concentrating on two WR+O systems, namely V444 Cygni, and HD 193793.

Type
Session IV. Binaries
Information
Symposium - International Astronomical Union , Volume 143: Wolf–Rayet Stars and Interrelations with other Massive Stars in Galaxies , 1991 , pp. 253
Copyright
Copyright © Kluwer 1991 

References

Williams, P., et al. 1990. M.N.R.A.S., 243, 662.Google Scholar