Mass transfer in TV Cassiopeiae

dc.contributor.author	Chaubey, U. S.
dc.date.accessioned	2011-01-11T07:05:23Z
dc.date.available	2011-01-11T07:05:23Z
dc.date.issued	1979
dc.identifier.citation	This article is taken from ADS database	en_US
dc.identifier.uri	http://hdl.handle.net/123456789/781
dc.description.abstract	The period variations of TV Cassiopeiae between 1901 and 1977 are discussed in the light of the period change model proposed by Biermann and Hall. During each period decrease 4.0 x 10¯⁶M☉ of mass is transferred from the secondary star to the primary. The average observable mass transfer rate is found to be 4.3 x 10¯⁷M☉ yr¯¹. This average rate corresponds to the thermal time-scale of the mass-losing star.	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	ass63-247
dc.subject	TV Cassiopeiae	en_US
dc.title	Mass transfer in TV Cassiopeiae	en_US
dc.type	Article	en_US