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The Radio Properties of Symbiotic Stars

Published online by Cambridge University Press:  12 April 2016

E.R. Seaquist
E.R. Seaquist*
Affiliation:
Department of Astronomy, University of TorontoToronto, Ontario, CanadaM5S 1A7

Abstract

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Radio thermal bremsstrahlung emission has now been detected at centimeter wavelengths from about thirty symbiotic stars. These data combined with optical and IR data show that the radio emission in most systems may be understood in terms of the ionization of part of the wind of a red giant by a hot companion. The radio properties of symbiotic stars are reviewed and the agreement with and the limitations of this picture are examined.

Type
Session 1. The Basic Data
Information
International Astronomical Union Colloquium , Volume 103: The Symbiotic Phenomenon , 1988 , pp. 69 - 75
Copyright
Copyright © Kluwer 1988

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