Distribution of bhb-stars in the cluster ω centauri and its effect on the radial change in colour and ellipticity of the cluster

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4864

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DC Field	Value	Language
dc.contributor.author	Scaria, K. K	-
dc.contributor.author	Bappu, M. K. V	-
dc.date.accessioned	2009-10-16T11:04:02Z	-
dc.date.available	2009-10-16T11:04:02Z	-
dc.date.issued	1984	-
dc.identifier.citation	Hidayat, B and Feast, M. W eds., Proceedings of the Second Asian Pacific Regional Meeting on Astronomy Bandung, Indonesia, 24 - 29 August, 1981, pp. 449 - 459	en
dc.identifier.uri	http://hdl.handle.net/2248/4864	-
dc.description.abstract	The authors have studied the radial change in the distribution of giant branch stars and the horizontal branch stars in ω Centauri. They show how the observed change in the distribution is related to the radial change in the colour of the cluster and also the radial change in its ellipticity.	en
dc.language.iso	en	en
dc.publisher	Tira Pustaka, Jakarta	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1984aprm.conf..449S	en
dc.rights	© International Astronomical Union	en
dc.subject	Galactic Structure	en
dc.subject	Stars Binary	en
dc.subject	Pulsars	en
dc.title	Distribution of bhb-stars in the cluster ω centauri and its effect on the radial change in colour and ellipticity of the cluster	en
dc.type	Article	en
Appears in Collections:	IIAP Publications

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