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Radio Imaging of Symbiotic Stars

Published online by Cambridge University Press:  12 April 2016

A.R. Taylor
A.R. Taylor*
Affiliation:
Department of Physics, University of Calgary Calgary, Alberta, Canada

Abstract

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A brief review of radio observations of individual symbiotic stars is presented, with emphasis on radio imaging of the circumstellar nebulae. The ionized nebulae are catagorized into two types: outburst ejecta and stellar winds. Among the ejecta-type there is a strong tendency for bipolar or jet morphology. In the case of the quiescent, stellar wind emitter, a few very wide binary systems (eg. Hl-36) offer the potential of directly viewing the effects of the binary interaction.

Type
Session 1. The Basic Data
Information
International Astronomical Union Colloquium , Volume 103: The Symbiotic Phenomenon , 1988 , pp. 77 - 83
Copyright
Copyright © Kluwer 1988

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