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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2275
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dc.contributor.authorHasan, P-
dc.contributor.authorKilambi, G. C-
dc.contributor.authorBaliyan, K. S-
dc.date.accessioned2008-05-08T09:50:54Z-
dc.date.available2008-05-08T09:50:54Z-
dc.date.issued2001-
dc.identifier.citationBASI, Vol. 29, No. 3, pp. 329 - 333en
dc.identifier.urihttp://hdl.handle.net/2248/2275-
dc.description.abstractIn an attempt to understand early phases of stellar evolution and star formation, we have taken up the study of extremely young star clusters in the near infrared wavebands. These clusters are deeply embedded inside the molecular gas and dust but radiate substantially in the infrared. We have observed one such cluster NGC 2453 from Mt Abu Infrared Observatory (MIRO) operated by the Physical Research Laboratory, using the NICMOS-3 infrared array mounted on the 1.2 m Cassegrain focus telescope. The observations were made in the J, H and K' wavebands in February 2000. The data reduction and the photometry has been performed using IRAF. Preliminary results are presented.en
dc.format.extent365433 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/2001BASI...29..329Hen
dc.subjectNICMOS cameraen
dc.subjectOpen clustersen
dc.subjectNear-infrareden
dc.subjectCluster distanceen
dc.titleNear IR study of the young cluster NGC 2453en
dc.typeArticleen
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