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The Structure of Colliding Stellar Winds

Published online by Cambridge University Press:  03 August 2017

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

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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
Copyright
Copyright © Kluwer 1991 

References

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