UBV photometry of ER Vulpeculae

dc.contributor.author	Srivastava, R. K.
dc.contributor.author	Padalia, T. D.
dc.contributor.author	Srivastava, J. B.
dc.date.accessioned	2010-01-18T10:18:17Z
dc.date.available	2010-01-18T10:18:17Z
dc.date.issued	1991
dc.identifier.citation	This article downloded from ADS Free Online Journal	en_US
dc.identifier.uri	http://hdl.handle.net/123456789/452
dc.description.abstract	UBV photometry of RS CVn- type eclipsing binary system ER Vulpeculae has been presented. The period comes out to be 0.ᵈ698093. The average depths of primary and secondary minima are, respectively,0.ᵐ21 and 0.ᵐ12. The colours at various phases have been given. A dip is seen around phase 0.ᵖ73 as was seen in the observations of Arevalo et al. (1988). Large scatter is present in the observations as noticed earlier, and may be due to activity of the components.	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	ass182-281
dc.subject	ER Vulpeculae	en_US
dc.title	UBV photometry of ER Vulpeculae	en_US
dc.type	Article	en_US