Variability of the hotter component of the eclipsing binary MM Cassiopeiae

dc.contributor.author	Chaubey, U. S.
dc.date.accessioned	2010-07-07T06:36:22Z
dc.date.available	2010-07-07T06:36:22Z
dc.date.issued	1983
dc.identifier.citation	This article is downloaded from ADS site	en_US
dc.identifier.uri	http://hdl.handle.net/123456789/693
dc.description.abstract	The eclipsing binary MM Cas (alpha_1980 = 0h53.4m and delta_1980 = +54d20.5') was observed photoelectrically during 13 nights from December 1980 to September 1982 with the 104 cm telescope of the Uttar Pradesh State Observatory to obtain the full UBV light curves. The telescope was equipped with a refrigerated EMI 6094S photomultiplier and standard UBV filters. The light curve obtained in V filter is given in Figure 1, the phases have been computed according to the ephemeris:	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	ibvs2348
dc.subject	Eclipsing Binary MM Cassiopeiae	en_US
dc.title	Variability of the hotter component of the eclipsing binary MM Cassiopeiae	en_US
dc.type	Article	en_US