CCD photometry of the galactic open star cluster-II. NGC 7419

dc.contributor.author	Bhatt, B. C.
dc.contributor.author	Pandey, A. K.
dc.contributor.author	Mohan, V.
dc.contributor.author	Mahra, H. S.
dc.contributor.author	Paliwal, D. C.
dc.date.accessioned	2010-01-13T10:51:31Z
dc.date.available	2010-01-13T10:51:31Z
dc.date.issued	1992
dc.identifier.uri	http://hdl.handle.net/123456789/425
dc.description.abstract	CCD photometric observations of open cluster NGC 7419 in UBVRI passbands have been made down to V= 19.5 mag. Reddening across the cluster region is found to be variable. The mean visual absorption of 5.30 mag and a distance of 2 kpc have been estimated for the cluster. The cluster age has been estimated to be nearly 40 Myr and less than 40 Myr, using the convective core overshooting isochrones and empirical isochrones respectively.	en_US
dc.language.iso	en	en_US
dc.relation.ispartofseries	basi21-33
dc.subject	Open Cluster, Photometry	en_US
dc.title	CCD photometry of the galactic open star cluster-II. NGC 7419	en_US
dc.type	Article	en_US