Photoelectric observations and the wave minimum of RS CVn

dc.contributor.author	Srivastava, R. K.
dc.date.accessioned	2010-02-18T06:58:55Z
dc.date.available	2010-02-18T06:58:55Z
dc.date.issued	1987
dc.identifier.citation	This article is downloaded for ADS	en_US
dc.identifier.uri	http://hdl.handle.net/123456789/551
dc.description.abstract	B, V observations of the eclipsing binary RS CVn have been presented. A dip around 0.ᴾ1 appears to be a wave minimum which fits well in the 'Wave minimum phase-time' relation, but deviates from the 'Wave aplitude-time' relation, derived for the RS CVn. Either, the 'Wave aplitude-time' requires a modification or the amplitude of the wave minmum appears masked by the intrinsic variability of one of the components or by the Sun-spot activity of the system. The colour exhibits variation. The secondary component appears active.	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	ass137-63
dc.subject	Eclipsing binary system RS CVn	en_US
dc.title	Photoelectric observations and the wave minimum of RS CVn	en_US
dc.type	Article	en_US