Spectrophotometric study of X Persei

dc.contributor.author	Sanwal, B. B.
dc.contributor.author	Rautela, B. S.
dc.contributor.author	Joshi, S. C.
dc.date.accessioned	2010-03-04T09:16:28Z
dc.date.available	2010-03-04T09:16:28Z
dc.date.issued	1985
dc.identifier.citation	This article is downloaded for ADS	en_US
dc.identifier.uri	http://hdl.handle.net/123456789/611
dc.description.abstract	The continuum energy distribution of the emission line star X Per (o9.5III-V) has been obtained in the wavelength range 340-710 nm and has been compared with the energy distribution of α Cam in the same wavelength range. The continuum of the star is found to be modified by the circumstellar envelop. A number density of the order of 10¹¹ in the envelop has been obtained from the observations of Hα in emission.	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	ass110-301
dc.subject	X Persei	en_US
dc.title	Spectrophotometric study of X Persei	en_US
dc.type	Article	en_US