Mass loss from Wolf-Rayet stars

dc.contributor.author	Singh, M.
dc.contributor.author	Chaubey, U. S.
dc.date.accessioned	2010-02-11T09:30:44Z
dc.date.available	2010-02-11T09:30:44Z
dc.date.issued	1986
dc.identifier.uri	http://hdl.handle.net/123456789/502
dc.description.abstract	The observed times of minimum light derived from the photometry of the Wolf-Rayet eclipsing binary stars CQ Ceq and V444 Cyg are used to estimated the mass-loss rate of the Wolf-Rayet components in several modes of mass-loss and mass-exchange.	en_US
dc.language.iso	en	en_US
dc.relation.ispartofseries	apss124-389
dc.subject	Wolf-Rayet stars	en_US
dc.title	Mass loss from Wolf-Rayet stars	en_US
dc.type	Article	en_US