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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2537
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dc.contributor.authorMathew, Annamma-
dc.contributor.authorRajamohan, R-
dc.date.accessioned2008-06-30T05:35:17Z-
dc.date.available2008-06-30T05:35:17Z-
dc.date.issued1992-03-
dc.identifier.citationJournal of Astrophysics and Astronomy, Vol. 13, No. 1, pp. 61 - 107en
dc.identifier.issn0250-6335-
dc.identifier.urihttp://hdl.handle.net/2248/2537-
dc.description.abstractThe observed uvby and H-beta indices of member stars of the Hyades and Praesepe clusters are analyzed in detail for rotation. The slopes of the rotation effects observed are utilized to determine the zero rotation main sequence (ZRMS) values of the intermediate band photometric indices for selected clusters. A preliminary calibration of the absolute visual magnitudes as a function of beta valid for zero rotation zero age main sequence (ZRZAMS) is deriveden
dc.format.extent3276376 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherIndian Academy of Sciencesen
dc.relation.urihttp://adsabs.harvard.edu/abs/1992JApA...13...61Men
dc.subjectMain sequence starsen
dc.subjectStar clustersen
dc.subjectStellar coloren
dc.subjectStellar rotationen
dc.subjectB starsen
dc.subjectInterstellar extinctionen
dc.subjectStellar luminosityen
dc.subjectStellar spectrophotometryen
dc.subjectUBV spectraen
dc.titleEffects of rotation on the colours and line indices of stars. V - The ZRMS and the ZRZAMSen
dc.typeArticleen
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