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Effects of rotation on the colours and line indices of stars. VI - The reality of the blue straggler phenomenon

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dc.contributor.author D'Souza, J
dc.contributor.author Mathew, Annamma
dc.contributor.author Rajamohan, R
dc.date.accessioned 2008-06-30T05:50:09Z
dc.date.available 2008-06-30T05:50:09Z
dc.date.issued 1992-03
dc.identifier.citation Journal of Astrophysics and Astronomy, Vol. 13, No. 1, pp. 109 - 128 en
dc.identifier.issn 0250-6335
dc.identifier.uri http://hdl.handle.net/2248/2538
dc.description.abstract The 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 alone en
dc.format.extent 1407775 bytes
dc.format.mimetype application/pdf
dc.language.iso en en
dc.publisher Indian Academy of Sciences en
dc.relation.uri http://adsabs.harvard.edu/abs/1992JApA...13..109D en
dc.subject B stars en
dc.subject Blue stars en
dc.subject Main sequence stars en
dc.subject Star clusters en
dc.subject Stellar color en
dc.subject Stellar rotation en
dc.subject A stars en
dc.subject Color-color diagram en
dc.subject Color-magnitude diagram en
dc.subject Interstellar extinction en
dc.title Effects of rotation on the colours and line indices of stars. VI - The reality of the blue straggler phenomenon en
dc.type Article en


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