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Radio and infrared emission by O-type and related stars

Published online by Cambridge University Press:  14 August 2015

M. J. Barlow
M. J. Barlow*
Affiliation:
Anglo-Australian Observatory, P.O. Box 296, Epping, N.S.W. 2121, Australia

Extract

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In addition to O-type stars, this review will discuss the radio and infrared properties of B supergiants and Wolf-Rayet stars, since it is generally accepted that these objects represent later stages in the evolution of O stars. The radio properties of X-ray binaries which exhibit non-thermal emission will not be discussed. Hjellming (1977) gives an excellent review of the radio properties of close binaries, including X-ray binaries.

Type
Session 3: Infrared and Radio Data
Information
Symposium - International Astronomical Union , Volume 83: Mass Loss and Evolution of O-Type Stars , 1979 , pp. 117 - 130
Copyright
Copyright © Reidel 1979 

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