Long-term study of the starspot activity on the eclipsing short-period RS Canum Venaticorum binary UV Piscium

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2273

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DC Field	Value	Language
dc.contributor.author	Radhika, P	-
dc.contributor.author	Vivekananda Rao, P	-
dc.date.accessioned	2008-05-08T09:21:48Z	-
dc.date.available	2008-05-08T09:21:48Z	-
dc.date.issued	2001	-
dc.identifier.citation	BASI, Vol. 29, No. 3, pp. 317 - 322	en
dc.identifier.uri	http://hdl.handle.net/2248/2273	-
dc.description.abstract	We present optical photometry of the short-period eclipsing RS CVn system, UV Piscium for the years 1966-1984. For each light curve, we model the distortion waves in order to study the behaviour of starspots in this system. After removing the spot effects from the light curves, we model the cleaned data to obtain system parameters. We also note changes in the luminosity of the primary star that are not explained by the spot variation.	en
dc.format.extent	526026 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.relation.uri	http://adsabs.harvard.edu/abs/2001BASI...29..317R	en
dc.subject	Optical photometry	en
dc.subject	UV Piscium	en
dc.subject	Starspots	en
dc.subject	RS Canum	en
dc.title	Long-term study of the starspot activity on the eclipsing short-period RS Canum Venaticorum binary UV Piscium	en
dc.type	Article	en
Appears in Collections:	BASI Publications

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