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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3652
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dc.contributor.authorMathew, A-
dc.contributor.authorRajamohan, R-
dc.date.accessioned2008-09-16T14:25:21Z-
dc.date.available2008-09-16T14:25:21Z-
dc.date.issued1990-06-
dc.identifier.citationJournal of Astrophysics and Astronomy, Vol. 11, No. 2, pp. 167 - 191en
dc.identifier.issn0250-6335-
dc.identifier.urihttp://hdl.handle.net/2248/3652-
dc.description.abstractThe intrinsic uvby and H-beta indices of member stars of Alpha-Persei, Pleiades, and Scorpio-Centaurus association have been analyzed in detail for rotation effects. These stars range in spectral type from B0 to F0 and the observed effects of rotation are found to be in agreement with photometric effects calculated by Collins and Sonneborn (1977) for rigidly rotating B0 to F0 stars.en
dc.language.isoenen
dc.publisherIndian Academy of Sciencesen
dc.relation.urihttp://cdsads.u-strasbg.fr/abs/1990JApA...11..167Men
dc.subjectH beta lineen
dc.subjectLine spectraen
dc.subjectStellar coloren
dc.subjectStellar rotationen
dc.subjectStellar spectraen
dc.subjectUBV spectraen
dc.subjectA starsen
dc.subjectB starsen
dc.subjectInterstellar extinctionen
dc.subjectStar clustersen
dc.subjectStellar spectrophotometryen
dc.titleEffects of rotation on the colours and line indices of stars. II - The effect on UVBY and H-beta indicesen
dc.typeArticleen
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