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UBV photometry of ER Vulpeculae

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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


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