Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3818
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dc.contributor.authorBabu, G. S. D-
dc.date.accessioned2008-09-23T11:33:14Z-
dc.date.available2008-09-23T11:33:14Z-
dc.date.issued1985-03-
dc.identifier.citationJournal of Astrophysics and Astronomy, Vol. 6, No. 1, pp. 61 - 70en
dc.identifier.issn0250-6335-
dc.identifier.urihttp://hdl.handle.net/2248/3818-
dc.description.abstractThe results of modified objective grating observations and photoelectric as well as photographic photometry of the open cluster NGC 2374 are presented. The cluster contains at least twenty stars as definite members down to mv ≈ 15 mag. There is a uniform extinction of E(B-V) = 0.175 mag and the distance is 1.2±0.1 kpc. The most likely age of this cluster is 7.5×10/sup7years.en
dc.language.isoenen
dc.publisherIndian Academy of Sciencesen
dc.relation.urihttp://ads.ari.uni-heidelberg.de/abs/1985JApA....6...61Ben
dc.subjectAstronomical Photometryen
dc.subjectOpen Clustersen
dc.subjectAstronomical Photographyen
dc.subjectDistanceen
dc.subjectElectrophotometryen
dc.subjectInterstellar Extinctionen
dc.subjectStellar Evolutionen
dc.subjectStellar Spectraen
dc.titleA study of the open cluster NGC 2374en
dc.typeArticleen
Appears in Collections:IIAP Publications

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