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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2278
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dc.contributor.authorGanesh, S-
dc.contributor.authorJoshi, U. C-
dc.contributor.authorBaliyan, K. S-
dc.contributor.authorShah, C. R-
dc.contributor.authorJain, J. K-
dc.contributor.authorRajpurohit, G. S-
dc.contributor.authorSanchawala, K-
dc.contributor.authorSaha, A. B-
dc.date.accessioned2008-05-08T11:19:04Z-
dc.date.available2008-05-08T11:19:04Z-
dc.date.issued2001-
dc.identifier.citationBASI, Vol. 29, No. 3, pp. 339 - 342en
dc.identifier.urihttp://hdl.handle.net/2248/2278-
dc.description.abstractDue mainly to high extinction in optical, the structure of our galaxy, Milky Way, is not very well understood. The Galactic disk and bulge contain a host of heavily reddened open clusters which are deeply embedded within dark molecular clouds of dust and gas. The extremely young stellar objects in these clouds can provide important informations for the study of stellar evolution and star formation. We report near infrared photometric study of one such cloud, Lynds 1340 in the survey mode. The cloud contains several nebulous regions and is shown to harbour a young cluster RN07. The near IR study provides detailed information on the embedded sources.en
dc.format.extent287350 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/2001BASI...29..339Gen
dc.subjectNICMOS cameraen
dc.subjectDark cloudsen
dc.subjectStar forming regionsen
dc.subjectNear Infrareden
dc.subjectClustersen
dc.titlePRLNIC3 observations of star forming cloud L1340en
dc.typeArticleen
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