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PRLNIC3 observations of star forming cloud L1340

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dc.contributor.author Ganesh, S
dc.contributor.author Joshi, U. C
dc.contributor.author Baliyan, K. S
dc.contributor.author Shah, C. R
dc.contributor.author Jain, J. K
dc.contributor.author Rajpurohit, G. S
dc.contributor.author Sanchawala, K
dc.contributor.author Saha, A. B
dc.date.accessioned 2008-05-08T11:19:04Z
dc.date.available 2008-05-08T11:19:04Z
dc.date.issued 2001
dc.identifier.citation BASI, Vol. 29, No. 3, pp. 339 - 342 en
dc.identifier.uri http://hdl.handle.net/2248/2278
dc.description.abstract Due 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.extent 287350 bytes
dc.format.mimetype application/pdf
dc.language.iso en en
dc.publisher Astronomical Society of India en
dc.relation.uri http://adsabs.harvard.edu/abs/2001BASI...29..339G en
dc.subject NICMOS camera en
dc.subject Dark clouds en
dc.subject Star forming regions en
dc.subject Near Infrared en
dc.subject Clusters en
dc.title PRLNIC3 observations of star forming cloud L1340 en
dc.type Article en


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