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Wolf-Rayet Binaries: Observational Aspects

Published online by Cambridge University Press:  03 August 2017

A. M. Cherepashchuk
A. M. Cherepashchuk*
Affiliation:
Sternberg Astronomical Institute Moscow University 119899, Universitetsky Prospect 13, Moscow, USSR

Abstract

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New data concerning observational aspects of Wolf-Rayet binaries are summarised. WR+O and WR+c binary systems are considered. All the data concerning WR binaries agree well with the modern understanding of WR stars as the helium remnants formed as a result of mass loss by massive O-type stars.

Type
Session IV. Binaries
Information
Symposium - International Astronomical Union , Volume 143: Wolf–Rayet Stars and Interrelations with other Massive Stars in Galaxies , 1991 , pp. 187 - 200
Copyright
Copyright © Kluwer 1991 

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