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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/353
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dc.contributor.authorScaria, K. K-
dc.date.accessioned2005-02-09T06:37:15Z-
dc.date.available2005-02-09T06:37:15Z-
dc.date.issued1982-12-
dc.identifier.citationBASI, Vol. 10, No. 4, pp. 340 - 347en
dc.identifier.urihttp://hdl.handle.net/2248/353-
dc.descriptionOpen Access-
dc.description.abstractIntegrated magnitudes in U, B, V, R and I bands are calculated for the globular cluseter Omega Centauri. The observed radial chaange in the integrated colour of the cluster shows that the cluster core (r<2') is redder in R - I colour and blure in U - B colour. It is argued that there is an increase in the ratio of AGB stars to the red gaints towards the centre of the cluster.en
dc.format.extent696091 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoen-
dc.publisherAstronomical Society of Indiaen
dc.subjectIntegrated Brightnessen
dc.subjectGlobular Clusteren
dc.subjectOmega Centaurien
dc.titleIntegrated brightness and colour of Omega Centaurien
dc.typeArticleen
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