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The Structure of the Circumstellar Material in Be Stars

Published online by Cambridge University Press:  26 May 2016

L.B.F.M. Waters  and
J.M. Marlborough
L.B.F.M. Waters
Affiliation:
Astronomical Institute Anton Pannekoek University of Amsterdam, Kruislaan 403, 1098 SJ Amsterdam SRON Laboratory for Space Research Groningen, P.O. Box 800, 9700 AV Groningen
J.M. Marlborough
Affiliation:
Astronomy Department, University of Western Ontario London, Ontario N6A 3K7, Canada

Abstract

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We review observations that are relevant for the determination of the structure and geometry of the circumstellar envelopes of Be stars. Evidence is summarized suggesting that Be stars have rotating discs. Infrared and radio continuum and line measurements and their interpretation are discussed.

Type
6. Be Stars: Circumstellar Environment
Information
Symposium - International Astronomical Union , Volume 162: Pulsation, Rotation and Mass Loss in Early-Type Stars , 1994 , pp. 399 - 411
Copyright
Copyright © Kluwer 1994 

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