CCD photometry of the galactic open cluster NGC 2309

dc.contributor.author	Nilakshi
dc.contributor.author	Pandey, A. K.
dc.contributor.author	Mohan, V.
dc.date.accessioned	2009-11-30T08:51:48Z
dc.date.available	2009-11-30T08:51:48Z
dc.date.issued	1998
dc.identifier.citation	This article downloded from ADS Free Online Journal	en_US
dc.identifier.uri	http://hdl.handle.net/123456789/369
dc.description.abstract	The comparison between the observed HR diagram of the clusters and the isochrones computed by means of evolutionary models provides a test for stellar structure and evolution. To get fundamental information for above mentioned studies the knowledge of reddening, distance, age and other parameters is necessary which can be derived from the colour-magnitude diagrams (CMDs) and colour-colour diagram (CCDs) of the clusters.	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	basi26-555
dc.subject	NGC 2309, CCD Photometry	en_US
dc.title	CCD photometry of the galactic open cluster NGC 2309	en_US
dc.type	Article	en_US