Spectrophotometric observations of HR 8107

dc.contributor.author	Joshi, S. C.
dc.contributor.author	Ojha, D. K.
dc.contributor.author	Srivastava, J. B.
dc.date.accessioned	2010-02-16T04:36:31Z
dc.date.available	2010-02-16T04:36:31Z
dc.date.issued	1989
dc.identifier.citation	This article is downloaded from ADS	en_US
dc.identifier.uri	http://hdl.handle.net/123456789/518
dc.description.abstract	HR 8107, a reported new Be star, has been observed spectrophotometrically. The energy distribution curve of the star has been compared with those of other stars of similar spectral and luminosity types and model atmospheres. On the basis of comparison with model atmospheres an effective temperature has been assigned to the star.	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	jaa10-113
dc.subject	Be stars - energy distribution	en_US
dc.title	Spectrophotometric observations of HR 8107	en_US
dc.type	Article	en_US