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Mass loss from Wolf-Rayet stars

Show simple item record Singh, M. Chaubey, U. S. 2010-02-11T09:30:44Z 2010-02-11T09:30:44Z 1986
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

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