Integrated brightness and colour of Omega Centauri

dc.contributor.author	Scaria, K. K
dc.date.accessioned	2005-02-09T06:37:15Z
dc.date.available	2005-02-09T06:37:15Z
dc.date.issued	1982-12
dc.identifier.citation	BASI, Vol. 10, No. 4, pp. 340 - 347	en
dc.identifier.uri	http://hdl.handle.net/2248/353
dc.description	Open Access
dc.description.abstract	Integrated 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.extent	696091 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en
dc.publisher	Astronomical Society of India	en
dc.subject	Integrated Brightness	en
dc.subject	Globular Cluster	en
dc.subject	Omega Centauri	en
dc.title	Integrated brightness and colour of Omega Centauri	en
dc.type	Article	en