Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1475
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dc.contributor.authorBhatt, B. C-
dc.contributor.authorPandey, A. K-
dc.contributor.authorMohan, V-
dc.contributor.authorMahra, H. S-
dc.contributor.authorPaliwal, D. C-
dc.date.accessioned2007-04-13T10:08:16Z-
dc.date.available2007-04-13T10:08:16Z-
dc.date.issued1993-03-
dc.identifier.citationBASI, Vol. 21, No. 1, pp 33-45en
dc.identifier.urihttp://hdl.handle.net/2248/1475-
dc.description.abstractCCD 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 respectivelyen
dc.format.extent837497 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.subjectOpen clusteren
dc.titleCCD photometry of galactic open star clusters -- 2: NGC 7419en
dc.typeArticleen
Appears in Collections:BASI Publications

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