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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/345
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dc.contributor.authorKilambi, G. C-
dc.date.accessioned2005-02-09T04:30:34Z-
dc.date.available2005-02-09T04:30:34Z-
dc.date.issued1982-09-
dc.identifier.citationBASI, Vol. 10, No. 3, pp. 234-243en
dc.identifier.urihttp://hdl.handle.net/2248/345-
dc.description.abstractAn analysis of UBV light variations of BS Aqr is presented. Intrinsic (U-B) and (B-V) values are used to derive the temperature and surface gravity. The mean values are Teff = 7600 + or - 100 K and log geff = 3.8 + or - 0.1. These values suggest that BS Aqr is a normal population I pulsating star and a member of Delta-Scuti group.en
dc.format.extent709799 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoen-
dc.publisherAstronomical Society of Indiaen
dc.subjectvariable staren
dc.subjectphotometryen
dc.subjectpulsationen
dc.subjectdwarf Cepheiden
dc.titleAnalysis of the light variations of BS Aquariien
dc.typeArticleen
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