Spectrophotometric observations of B type stars HR 1207 and HR 1770

dc.contributor.author	Joshi, S. C.
dc.contributor.author	Ojha, D. K.
dc.date.accessioned	2010-01-15T05:35:37Z
dc.date.available	2010-01-15T05:35:37Z
dc.date.issued	1991
dc.identifier.citation	This article downloded from ADS Free Online Journal	en_US
dc.identifier.uri	http://hdl.handle.net/123456789/437
dc.description.abstract	Two high rotational velocity B type stars HR 1207 and HR 1770 have been observed spectrophotometrically. The energy distribution curves of the stars have been compared with model atmospheres in the ultraviolet and visible regions. Temperature estimates with different methods are made and certain peculiarities in the energy distribution curves of the stars discussed.	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	basi19-53
dc.subject	B stars, Be Stars, Energy distribution	en_US
dc.title	Spectrophotometric observations of B type stars HR 1207 and HR 1770	en_US
dc.type	Article	en_US