CCD photometry of galactic open star clusters -- 2: 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	2007-04-13T10:08:16Z
dc.date.available	2007-04-13T10:08:16Z
dc.date.issued	1993-03
dc.identifier.citation	BASI, Vol. 21, No. 1, pp 33-45	en
dc.identifier.uri	http://hdl.handle.net/2248/1475
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
dc.format.extent	837497 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.subject	Open cluster	en
dc.title	CCD photometry of galactic open star clusters -- 2: NGC 7419	en
dc.type	Article	en