Mass transfer in algols and its implications to the mass transfer theory

dc.contributor.author	Chaubey, U. S.
dc.date.accessioned	2010-01-12T08:34:02Z
dc.date.available	2010-01-12T08:34:02Z
dc.date.issued	1993
dc.identifier.uri	http://hdl.handle.net/123456789/420
dc.description.abstract	The average mass transfer rates in four Algol-type binary stars RZ Cas, TV Cas, SW Cyg and BI Peg are derived from their observed period changes in the light of alternate period change model. The results have been used to discuss the anomalies in the mass transfer theory, namely dynamical instability of the mass losing component and the conservation of orbital angular momentum during the mass transfer.	en_US
dc.language.iso	en	en_US
dc.relation.ispartofseries	basi21-597
dc.subject	Mass Transfer, Binaries	en_US
dc.title	Mass transfer in algols and its implications to the mass transfer theory	en_US
dc.type	Article	en_US