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Wolf-Rayet Stars with Compact Companions

Published online by Cambridge University Press:  14 August 2015

Anthony F.J. Moffat
Anthony F.J. Moffat*
Affiliation:
Département de physique, Université de Montréal

Abstract

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Evidence is accumulating in favour of a heretofore missing link in the evolution of massive binary stars — a second WR phase in which the companion to the WR star is a neutron star of mass 1–2 M⊙, or in some cases a more massive black hole. The discovery of such objects is also important in assessing the role of duplicity in the formation of WR stars.

Type
SESSION 4 — OBSERVATIONS OF WOLF-RAYET BINARIES
Information
Symposium - International Astronomical Union , Volume 99: Wolf-Rayet Stars: Observations, Physics, Evolution , 1982 , pp. 263 - 275
Copyright
Copyright © Reidel 1982 

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