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The Environments of Cool Stars

Published online by Cambridge University Press:  12 April 2016

Robert E. Stencel
Robert E. Stencel*
Affiliation:
Center for Astrophysics and Space Astronomy, University of ColoradoBoulder, CO 80309-0391, USA

Abstract

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This review describes recent conclusions about the physical environment of red giant and supergiant stars. This includes coronae, chromospheres, dust formation and stellar winds. This knowledge can provide the boundary conditions for considering what role such objects play as members of binary star systems, where tidal forces and companion behavior alter observed characteristics.

Type
Session 1. The Basic Data
Information
International Astronomical Union Colloquium , Volume 103: The Symbiotic Phenomenon , 1988 , pp. 57 - 64
Copyright
Copyright © Kluwer 1988

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