Spectrophotometric observations and evolutionary status of ten Be stars

dc.contributor.author	Singh, M.
dc.contributor.author	Chaubey, U. S.
dc.date.accessioned	2010-02-25T06:48:27Z
dc.date.available	2010-02-25T06:48:27Z
dc.date.issued	1987
dc.identifier.citation	This article is downloaded for ADS	en_US
dc.identifier.uri	http://hdl.handle.net/123456789/584
dc.description.abstract	The continuum energy distribution data of ten Be stars - namely, HR 1761, HR 1786, HR 1820, σOri, ω Ori, OT Gem, β Lyr, HR 7983, νCyg, and 59 Cyg- have been presented in the wavelength range λλ3200-8000 Å. The observed energy distribution curve shows near infrared excess for majority of Be stars and a double Balmer jump for HR 8047 and HR 8146. Empirical effective temperatures of these stars have been estimated by comparing the observed continuum energy distribution with that of computed theoretical models given by Kurucz (1979).	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	ass129-251
dc.subject	Be stars	en_US
dc.title	Spectrophotometric observations and evolutionary status of ten Be stars	en_US
dc.type	Article	en_US