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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1923
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dc.contributor.authorKarnik, A. D-
dc.contributor.authorGhosh, S. K-
dc.contributor.authorRengarajan, T. N-
dc.contributor.authorTandon, S. N-
dc.contributor.authorVerma, R. P-
dc.date.accessioned2007-10-24T11:56:02Z-
dc.date.available2007-10-24T11:56:02Z-
dc.date.issued1999-
dc.identifier.citationBASI, Vol. 27, No. 1, pp. 167 - 170en
dc.identifier.urihttp://hdl.handle.net/2248/1923-
dc.description.abstractStar forming regions associated with IRAS 19181+1349, 20255+3712, 20178+4046 and 10049+5657 have been mapped simultaneously in two far infrared bands (λeff ~ 130 and 210 µm), using TIFR 1m balloon borne telescope with liquid 3He cooled bolometer arrays. HIRES processed IRAS maps at 12, 25, 60 and 100 µm have been compared with ours. The TIFR maps show much more structural details due to their superior angular resolution. Detail radiation transfer modelling has been carried out for each of these sources and compared with observed spectral energy distributions.en
dc.format.extent269088 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/1999BASI...27..167Ken
dc.subjectInfrared emissionen
dc.subjectStar formationen
dc.subjectMolecular clouden
dc.titleInfrared spectral energy distribution of four star forming regionsen
dc.typeArticleen
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