Spectrophotometric observations of UX Arietis

dc.contributor.author	Joshi, S. C.
dc.contributor.author	Srivastava, R. K.
dc.contributor.author	Srivastava, J. B.
dc.date.accessioned	2010-01-18T08:45:24Z
dc.date.available	2010-01-18T08:45:24Z
dc.date.issued	1991
dc.identifier.citation	This article downloded from ADS Free Online Journal	en_US
dc.identifier.uri	http://hdl.handle.net/123456789/451
dc.description.abstract	Spectrophotometric observations of the RS Cvn binary UX Arietis have been presented. The comparison of the observed fluxes with model atmospheres indicates that during the four phases observed, the temperature does not vay significantly. However, brightness variation of 0.ᵐ23 are thought to be due to change in the surface emitting regions.	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	ass183-11
dc.subject	UX Arietis	en_US
dc.title	Spectrophotometric observations of UX Arietis	en_US
dc.type	Article	en_US