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Evolution of massive close binaries, compared to observations

Published online by Cambridge University Press:  25 May 2016

Dany Vanbeveren
Dany Vanbeveren*
Affiliation:
Astrophysical Institute, Vrije Universiteit Brussel, Pleinlaan 2, B-1050 Brussels, Belgium

Abstract

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Since binaries can not be considered separately from single stars, we first present a brief summary of massive single star evolution. Next, we highlight massive close binary evolutionary facts that are important when massive close binaries are included in population (number) synthesis. Finally, we consider a few interesting test cases.

Type
Part 2. Models for single star evolution of massive stars: wind + atmosphere + interior
Information
Symposium - International Astronomical Union , Volume 193: Wolf-Rayet Phenomena in Massive Stars and Starburst Galaxies , 1999 , pp. 196 - 204
Copyright
Copyright © Astronomical Society of the Pacific 1999 

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