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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.identifier.citationBASI, Vol. 27, No. 1, pp. 155 - 158en
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.publisherAstronomical Society of Indiaen
dc.subjectInfrared emissionen
dc.subjectIRAS 00338+6312en
dc.subjectZAMS staren
dc.titleInfrared emission from IRAS 00338+6312en
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