Period study of the short period RS CVn type  eclipsing binary UV Piscium

dc.contributor.author	Vivekananda Rao, P
dc.contributor.author	Sarma, M. B. K
dc.date.accessioned	2005-12-05T07:23:06Z
dc.date.available	2005-12-05T07:23:06Z
dc.date.issued	1983-03
dc.identifier.citation	BASI, Vol. 11, No. 1, pp. 75-81	en
dc.identifier.uri	http://hdl.handle.net/2248/587
dc.description.abstract	The short period RS CVn type eclipsing binary UV Piscium was observed photoelectrically with standard U, B, V filters for three consecutive observing seasons during 1976-1979. A total of nine primary minima in each of V and B colours and seven primary minima in U colour were obtained. All these minima and those obtained by Carr, Oliver, and Sadik were corrected for the distortion wave superposed on the light curves. Using these wave-corrected times of minima the following improved light elements were derived : Hel. JD 2443080.1843 + 0/sopd/. 8610474 E. The (O -C)s obtained using these ephemeris suggest no earlier suggestions of period variation in this system.	en
dc.format.extent	477311 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en
dc.publisher	Astronomical Society of India	en
dc.subject	Period study - RS CVn type eclipsing binary	en
dc.subject	UV Piscium	en
dc.title	Period study of the short period RS CVn type eclipsing binary UV Piscium	en
dc.type	Article	en