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

dc.contributor.author	Chaubey, U. S
dc.date.accessioned	2007-05-10T05:33:53Z
dc.date.available	2007-05-10T05:33:53Z
dc.date.issued	1993
dc.identifier.citation	BASI, Vol. 21, pp. 597-600	en
dc.identifier.uri	http://hdl.handle.net/2248/1563
dc.description.abstract	he 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.extent	294030 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.subject	Mass trnasfer	en
dc.subject	Binaries	en
dc.title	Mass transfer in ALGOLS and its implications to the mass transfer theory	en
dc.type	Article	en