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Duplicity of Be Stars as Seen from Ondřejov: (Review Paper)
Published online by Cambridge University Press: 14 August 2015
Abstract
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.
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- Part VI: Single Versus Binary Stars
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- Copyright © Reidel 1976
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