CCD photometry of galactic open star clusters – V. King 7

dc.contributor.author	Durgapal, A. K.
dc.contributor.author	Pandey, A. K.
dc.contributor.author	Mohan, V.
dc.date.accessioned	2009-11-30T09:30:39Z
dc.date.available	2009-11-30T09:30:39Z
dc.date.issued	1997
dc.identifier.citation	This article downloded from ADS Free Online Journal	en_US
dc.identifier.uri	http://hdl.handle.net/123456789/373
dc.description.abstract	CCD observations of the open clusters King 7 and two nearby fields have been made in the UBVRI passbands down to V ~ 20.0 mag. From the colour-colour diagram the reddening is estimated to be 1.25 mag. Comparison of the observational colour-magnitude diagrams (CMDs) with the convective core overshoot models (Bertelli et al. 1994) produces a good fit for a metallicity Z = 0.008 and age of 0.6-0.8 Gyr. An apparent distance modules (m-M) of 15.6 has been estimated for King 7 which puts it at a distance of 2.2 ± 0.34 kpc from us.	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	basi25-489
dc.subject	Open cluster – photometry	en_US
dc.title	CCD photometry of galactic open star clusters – V. King 7	en_US
dc.type	Article	en_US