An anlysis of the light changes of the eclipsing binary XY Ceti in the frequency-domain

dc.contributor.author	Srivastava, R. K.
dc.date.accessioned	2010-02-18T06:38:20Z
dc.date.available	2010-02-18T06:38:20Z
dc.date.issued	1987
dc.identifier.citation	This article is downloaded for ADS	en_US
dc.identifier.uri	http://hdl.handle.net/123456789/549
dc.description.abstract	The photoelectric observations of the eclipsing binary XY Ceti presented by us (see Srivastava and Padalia, 1975) have been analysed by Okazaki (1978) and Ramella et al.(1980). They presented different sets of elements from the same set of our observations. The necessitated us to obtain the elements of XY Ceti again employing method of determination of elements. The revised geometrical elements of the eclipsing binary XY Ceti have been obtained by the method of Fourier analysis of the light changes in the frewuency-domain, which was developed by Kopal (1979). These have been compared with our earlier (Srivastava and Padalia, 1975) results obtained by employing Russell and Merrill's (1952) method.	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	ass138-197
dc.subject	Eclipsing binary XY Ceti	en_US
dc.title	An anlysis of the light changes of the eclipsing binary XY Ceti in the frequency-domain	en_US
dc.type	Article	en_US