Study of the open cluster NGC 2264

dc.contributor.author	Sagar, R.
dc.contributor.author	Joshi, U. C.
dc.date.accessioned	2010-07-15T06:39:55Z
dc.date.available	2010-07-15T06:39:55Z
dc.date.issued	1983
dc.identifier.citation	This article is downloaded from ADS site	en_US
dc.identifier.uri	http://hdl.handle.net/123456789/704
dc.description.abstract	Photoelectric UBV magnitudes and colours have been determined for 138 stars in NGC 2264, having membership probability greater than 50 per cent on the basis of proper motion studies. The reddening across the cluster is variable. The distance modulus to the cluster is estimated at 9.5 ± 0.2 mag.	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	mn205-747
dc.subject	NGC 2264	en_US
dc.title	Study of the open cluster NGC 2264	en_US
dc.type	Article	en_US