Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1563
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dc.contributor.authorChaubey, U. S-
dc.date.accessioned2007-05-10T05:33:53Z-
dc.date.available2007-05-10T05:33:53Z-
dc.date.issued1993-
dc.identifier.citationBASI, Vol. 21, pp. 597-600en
dc.identifier.urihttp://hdl.handle.net/2248/1563-
dc.description.abstracthe average mass transfer rates in four Algol-type binary stars RZ Cas, TV Cas, SW Cyg and DI 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
dc.format.extent294030 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.subjectMass trnasferen
dc.subjectBinariesen
dc.titleMass transfer in ALGOLS and its implications to the mass transfer theoryen
dc.typeArticleen
Appears in Collections:BASI Publications

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