Rapid variation in Hα emission of  γ Cassiopeiae

dc.contributor.author	Joshi, S. C.
dc.contributor.author	Srivastava, R. K.
dc.contributor.author	Srivastava, J. B.
dc.date.accessioned	2010-02-18T06:15:18Z
dc.date.available	2010-02-18T06:15:18Z
dc.date.issued	1987
dc.identifier.citation	This article is downloaded for ADS	en_US
dc.identifier.uri	http://hdl.handle.net/123456789/546
dc.description.abstract	The well known Be star γ Cassiopeiae has been an object of intense study through over a century. Apart form the major phases namely, Be, Be shell, and normal B star with time scales of decades, the star also shows rapid changes in the visible spectrum.	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	ibvs3116
dc.subject	Hα emission, Be star - γ Cassiopeiae	en_US
dc.title	Rapid variation in Hα emission of γ Cassiopeiae	en_US
dc.type	Article	en_US