Photometric elements of V364 Cassiopeiae

dc.contributor.author	Chaubey, U. S.
dc.date.accessioned	2010-03-04T09:43:40Z
dc.date.available	2010-03-04T09:43:40Z
dc.date.issued	1984
dc.identifier.citation	This article is downloaded for ADS	en_US
dc.identifier.uri	http://hdl.handle.net/123456789/615
dc.description.abstract	The UBV photometric observations of the eclipsing binary V364 Cas have been discussed. Two sets of photometric elements, one based on the Russell and Merrill methods and the other based on Kopal's new method of the analysis of the light curves of eclipsing binary stars in the frequency-domain, have been derived. Using the observed colour indices U-B and B-V, the spectral types of the systemic components are estimated. An examination of all the available times of minimum light of V364 Cas does not reveal any change in its orbital period.	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	ass106-273
dc.subject	Eclipsing binary V364 Cas	en_US
dc.title	Photometric elements of V364 Cassiopeiae	en_US
dc.type	Article	en_US