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Duplicity of Be Stars as Seen from Ondřejov: (Review Paper)

Published online by Cambridge University Press:  14 August 2015

Petr Harmanec  and
Svatopluk Kříž
Petr Harmanec
Affiliation:
Astronomical Institute of the Czechoslovak Academy of Sciences, Ondřejov, Czechoslovakia
Svatopluk Kříž
Affiliation:
Astronomical Institute of the Czechoslovak Academy of Sciences, Ondřejov, Czechoslovakia

Abstract

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Observed Be stars are considered to be interacting binaries undergoing mostly case B mass exchange. Their observed properties can be explained satisfactorily as the consequences of different modes of mass transfer. Suggestions for further observational and theoretical studies to verify or to disprove the hypothesis presented here are briefly outlined.

Type
Part VI: Single Versus Binary Stars
Information
Symposium - International Astronomical Union , Volume 70: Be and Shell Stars , 1976 , pp. 385 - 400
Copyright
Copyright © Reidel 1976 

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