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Structure and evolution of massive single stars and their relevance for close binary systems

Published online by Cambridge University Press:  07 August 2017

Norbert Langer
Norbert Langer*
Affiliation:
Max-Planck-Institut für Astrophysik, D-85740 Garching, B.R. Deutschland

Abstract

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Differences in the evolution of massive single stars and components of massive close binary systems are investigated. While for stars above the red supergiant luminosity limit, single star and case B primary evolution merge into a single scenario, large differences for less massive stars are demonstrated to occur at the example of MZAMS = 40M⊙, concerning the various WR subtypes, the nucleosynthesis yields, and the supernova stage.

Keywords

stars: Wolf-Rayetmassive starsevolutionbinary evolution
Type
Session I - Basic parameters, properties of single Wolf-Ray et stars
Information
Symposium - International Astronomical Union , Volume 163: Wolf-Rayet Stars: Binaries, Colliding Winds, Evolution , 1995 , pp. 15 - 23
Copyright
Copyright © Kluwer 1995 

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