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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/947
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dc.contributor.authorMohan, V-
dc.contributor.authorSagar, R-
dc.date.accessioned2006-04-11T08:30:11Z-
dc.date.available2006-04-11T08:30:11Z-
dc.date.issued1988-12-
dc.identifier.citationBASI, Vol. 16, No. 4, pp. 159-182en
dc.identifier.urihttp://hdl.handle.net/2248/947-
dc.description.abstractPhotographic photometry of about 900 stars down to V = 17 mag has been carried out in the region of the open cluster NGC 2301. The cluster region seems to be severely contaminated by field stars. Statistical criteria yield only 96 + or - 17 cluster members. Stars fainter than about 15 mag are found to be absent among cluster members. Star counts indicate a diameter of about 20 arcmin. The data suggest mass segregation in the clusteren
dc.format.extent1563664 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indianen
dc.subjectOpen clusteren
dc.subjectPhotographic photometryen
dc.subjectStar countsen
dc.titleField star contamination in open star cluster NGC 2301en
dc.typeArticleen
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