On the primary minimum of eclipsing binary AY Cam

dc.contributor.author	Srivastava, J. B.
dc.contributor.author	Kandpal, C. D.
dc.date.accessioned	2010-02-26T06:14:33Z
dc.date.available	2010-02-26T06:14:33Z
dc.date.issued	1987
dc.identifier.citation	This article is downloaded for ADS	en_US
dc.identifier.uri	http://hdl.handle.net/123456789/590
dc.description.abstract	The eclipsing binary AY Cam (= BV 363 = BD + 77° 0328) was discovered by Strohmeier and Knigge (1961). They assigned it a period of 1ͩ. 367485. The photographic light curve is of Algol type with no indication of secondary minimum, the range of light variation being 9ͫ.9-10ͫ.75. According to McDonald (1964) the spectral type of AY Cam is GO, while Gotz and Wenzel (1966) reported its spectral type as A5.	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	ibvs3005
dc.subject	Eclipsing binary AY Cam	en_US
dc.title	On the primary minimum of eclipsing binary AY Cam	en_US
dc.type	Article	en_US