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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2538
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dc.contributor.authorD'Souza, J-
dc.contributor.authorMathew, Annamma-
dc.contributor.authorRajamohan, R-
dc.date.accessioned2008-06-30T05:50:09Z-
dc.date.available2008-06-30T05:50:09Z-
dc.date.issued1992-03-
dc.identifier.citationJournal of Astrophysics and Astronomy, Vol. 13, No. 1, pp. 109 - 128en
dc.identifier.issn0250-6335-
dc.identifier.urihttp://hdl.handle.net/2248/2538-
dc.description.abstractThe effect of rotation on the observed colors of stars has been considered as a possible cause for the blue straggler phenomenon in clusters listed by Mermilliod (1982). It appears that this phenomenon is definitely not real in the case of the late B and early A spectral type blue stragglers that are intrinsic slow rotators. Among clusters containing the early B type blue stragglers it is found that the anomalous position of the stragglers in NGC 6633, NGC 4675, and NGC 2516 cannot be accounted for by rotation effects aloneen
dc.format.extent1407775 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherIndian Academy of Sciencesen
dc.relation.urihttp://adsabs.harvard.edu/abs/1992JApA...13..109Den
dc.subjectB starsen
dc.subjectBlue starsen
dc.subjectMain sequence starsen
dc.subjectStar clustersen
dc.subjectStellar coloren
dc.subjectStellar rotationen
dc.subjectA starsen
dc.subjectColor-color diagramen
dc.subjectColor-magnitude diagramen
dc.subjectInterstellar extinctionen
dc.titleEffects of rotation on the colours and line indices of stars. VI - The reality of the blue straggler phenomenonen
dc.typeArticleen
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