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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3757
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dc.contributor.authorMohin, S-
dc.contributor.authorRaveendran, A. V-
dc.date.accessioned2008-09-22T11:36:06Z-
dc.date.available2008-09-22T11:36:06Z-
dc.date.issued1987-12-
dc.identifier.citationJournal of Astrophysics and Astronomy , Vol. 8, No. 4, pp. 389 - 395en
dc.identifier.issn0250-6335-
dc.identifier.urihttp://hdl.handle.net/2248/3757-
dc.description.abstractBV photometry of HD 116204 have been obtained on 57 nights during the 1983-1984, 1984-1985, and 1986-1987 observing seasons with the 34-cm reflector of the Vainu Bappu Observatory in Kavalur. A photometric period of 21.9 + or - 0.2 d and a mean (B-V) of 1.196 + or - 0.010 have been determined, and a mass ratio close to unity for HD 116204 is implied. The results suggest a vertical shift of the entire light curve towards brighter magnitudes and a low inclination of the rotation axis.en
dc.language.isoenen
dc.publisherIndian Academy of Sciencesen
dc.relation.urihttp://adsabs.harvard.edu/abs/1987JApA....8..389Men
dc.subjectBinary starsen
dc.subjectStellar spectrophotometryen
dc.subjectUBV spectraen
dc.subjectVisual photometryen
dc.subjectLight curveen
dc.subjectMass ratiosen
dc.subjectStellar coloren
dc.subjectStellar magnitudeen
dc.subjectStellar massen
dc.subjectBV Photometryen
dc.subjectHD116204en
dc.subjectRS CVn Systemen
dc.titleThe RS Canum Venaticorum binary HD 116204en
dc.typeArticleen
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