Continuum energy distribution of some bright Be stars

dc.contributor.author	Goraya, P. S.
dc.date.accessioned	2010-03-10T06:44:16Z
dc.date.available	2010-03-10T06:44:16Z
dc.date.issued	1984
dc.identifier.citation	This article is downloaded for ADS	en_US
dc.identifier.uri	http://hdl.handle.net/123456789/627
dc.description.abstract	The absolute flux distribution of seven bright Be stars, in the wavelength λλ350-750 nm is presented. The observed energy distribution curves are compared with Kurucz (1979) model atmospheres to estimate their effective temperatures. Some peculiarities in the energy distributions and evolutionary stages of the Be stars are discussed.	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	aa138-19
dc.subject	Continuum energy distribution - Be stars	en_US
dc.title	Continuum energy distribution of some bright Be stars	en_US
dc.type	Article	en_US