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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/587
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dc.contributor.authorVivekananda Rao, P-
dc.contributor.authorSarma, M. B. K-
dc.date.accessioned2005-12-05T07:23:06Z-
dc.date.available2005-12-05T07:23:06Z-
dc.date.issued1983-03-
dc.identifier.citationBASI, Vol. 11, No. 1, pp. 75-81en
dc.identifier.urihttp://hdl.handle.net/2248/587-
dc.description.abstractThe 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.extent477311 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoen-
dc.publisherAstronomical Society of Indiaen
dc.subjectPeriod study - RS CVn type eclipsing binaryen
dc.subjectUV Pisciumen
dc.titlePeriod study of the short period RS CVn type eclipsing binary UV Pisciumen
dc.typeArticleen
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