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Binary Evolution in the Upper HRD

Published online by Cambridge University Press:  04 August 2017

J.P. De Greve  and
C. de Loore
J.P. De Greve
Affiliation:
Astrophysical Institute VUB Brussels, Belgium
C. de Loore
Affiliation:
Astrophysical Institute VUB Brussels, Belgium

Abstract

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The importance of close binaries in the domain of luminous objects is examined. The group of unevolved massive stars of O- and B-type, the groups of Wolf-Rayet binaries and X-ray binaries are discussed, and limits on the mass ratios, masses and periods are listed, as well as the average values. The connections between these various groups are investigated, and relations among subgroups are established.

Type
Session 5. Massive Star Evolution
Information
Symposium - International Astronomical Union , Volume 116: Luminous Stars and Associations in Galaxies , 1986 , pp. 339 - 352
Copyright
Copyright © Reidel 1986 

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