Continuum energy distribution of Be stars

dc.contributor.author	Singh, M.
dc.date.accessioned	2010-03-03T10:14:47Z
dc.date.available	2010-03-03T10:14:47Z
dc.date.issued	1985
dc.identifier.citation	This article is downloaded from ADS	en_US
dc.identifier.uri	http://hdl.handle.net/123456789/600
dc.description.abstract	The continuum energy distributions of four Be stars - namely, HR 7708, HR 7807, HR 7927, and HR 8171 alongwith two normal B stars HR 7426 and HR 7613 are presented in the wavelength region λλ3200-7800 Å. By a comparison the observed continum energy distributions with that of theoritical models given by Kurucz (1979), their effective temperatures are determined and discussed. The observed energy distribution curves show near infrared excess emission longward of λ6000 Å for HR 7807 and HR 8171 and a double Balmer jump for HR 7708.	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	ass113-325
dc.subject	Energy distribution - Be stars	en_US
dc.title	Continuum energy distribution of Be stars	en_US
dc.type	Article	en_US