Absolute energy distribution in Rho Cassiopeiae

dc.contributor.author	Joshi, S. C.
dc.contributor.author	Rautela, B. S.
dc.date.accessioned	2011-11-14T05:45:02Z
dc.date.available	2011-11-14T05:45:02Z
dc.date.issued	1978
dc.identifier.citation	This article is downloaded from ADS article service	en_US
dc.identifier.uri	http://hdl.handle.net/123456789/866
dc.description.abstract	The continuous energy distribution of ρ Cas obtained in the wavelength range 340-710 nm has beeb compared with the energy distribution of δ CMa in the same wavelength range. The circumstellar shell associated with ρ Cas seems to modify the continuum of the star appreciably. Vatiations in the Balmer emission of ρ Cas taking place within a day are noticed.	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	mn183-55
dc.subject	Rho Cassiopeiae	en_US
dc.title	Absolute energy distribution in Rho Cassiopeiae	en_US
dc.type	Article	en_US