Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1920
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dc.contributor.authorMookerjea, B-
dc.contributor.authorGhosh, S. K-
dc.contributor.authorKarnik, A. D-
dc.contributor.authorRengarajan, T. N-
dc.contributor.authorTandon, S. N-
dc.contributor.authorVerma, R. P-
dc.date.accessioned2007-10-24T09:03:25Z-
dc.date.available2007-10-24T09:03:25Z-
dc.date.issued1999-
dc.identifier.citationBASI, Vol. 27, No. 1, pp. 155 - 158en
dc.identifier.urihttp://hdl.handle.net/2248/1920-
dc.description.abstractThe Galactic star forming region associated with IRAS 00338+6312 has been mapped in 2 Far Infrared (FIR) bands centered around 140 & 185 μm, using the TIFR 100 cm balloon-borne telescope with liquid 3/sup He cooled bolometer arrays. The results from these observations and the physical parameters derived from radiation transfer modelling of the source are presented.en
dc.format.extent201211 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/1999BASI...27..155Men
dc.subjectInfrared emissionen
dc.subjectIRAS 00338+6312en
dc.subjectZAMS staren
dc.titleInfrared emission from IRAS 00338+6312en
dc.typeArticleen
Appears in Collections:BASI Publications

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