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Radio Evidence for Non-isotropic Outflows from Hot Stars

Published online by Cambridge University Press:  12 April 2016

Stephen White
Stephen White*
Affiliation:
Dept. of Astronomy, University of Maryland, College Park, MD20742

Abstract

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Radio diagnostics for outflows from hot stars are reviewed and three well–studied examples (WR 140, η Car and MWC 349) are discussed in some detail. The three systems are very different and their radio properties are diverse, but in each case, the radio data provide strong evidence for the presence of equatorially–enhanced outflows.

Type
Section I Observations of Non-spherical Winds
Information
International Astronomical Union Colloquium , Volume 169: Variable and Non-spherical Stellar Winds in Luminous Hot Stars , 1999 , pp. 80 - 86
Copyright
Copyright © Springer-Verlag 1999

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