Spectrophotometry of some Be Stars

dc.contributor.author	Singh, M.
dc.date.accessioned	2010-02-09T05:53:12Z
dc.date.available	2010-02-09T05:53:12Z
dc.date.issued	1986
dc.identifier.uri	http://hdl.handle.net/123456789/494
dc.description.abstract	The continuum energy distributions of six Be stars, namely 25 Cyg, 31 Peg, HR 8758, 14 Lac, 12 Vul and β Psc in the wavelength region λ λ3200-7800 Å, are presented. Comparing the observed energy distributions with those of theoretical models given by Kurucz (1979), their effective temperatures are determined. A near-infrared excess emission at wavelengths above λ6000 Å is seen in most of the stars.	en_US
dc.language.iso	en	en_US
dc.relation.ispartofseries	apss120-133
dc.subject	Be Stars, Spectrophotometry	en_US
dc.title	Spectrophotometry of some Be Stars	en_US
dc.type	Article	en_US