Spectrophotometry of bright Be stars

dc.contributor.author	Goraya, P. S.
dc.date.accessioned	2010-03-04T06:47:16Z
dc.date.available	2010-03-04T06:47:16Z
dc.date.issued	1985
dc.identifier.citation	This article is downloaded for ADS	en_US
dc.identifier.uri	http://hdl.handle.net/123456789/607
dc.description.abstract	We present new measurement of the distribution of energy in the continuum for eight Be stars in the optical region (λλ3200-7600Å). The effective temperatures of these stars have been estimated from their observed fluxes. It is found that, in general, 'pole-on' stars show near-infrared excess emission,. It is interesting to note the Balmer jumps for stars having an infrared excess are systematically smaller than for those lacking the infrared excess.	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	ass112-1
dc.subject	Be stars - spectrophotometry	en_US
dc.title	Spectrophotometry of bright Be stars	en_US
dc.type	Article	en_US