Infrared spectral energy distribution of four star forming regions

dc.contributor.author	Karnik, A. D
dc.contributor.author	Ghosh, S. K
dc.contributor.author	Rengarajan, T. N
dc.contributor.author	Tandon, S. N
dc.contributor.author	Verma, R. P
dc.date.accessioned	2007-10-24T11:56:02Z
dc.date.available	2007-10-24T11:56:02Z
dc.date.issued	1999
dc.identifier.citation	BASI, Vol. 27, No. 1, pp. 167 - 170	en
dc.identifier.uri	http://hdl.handle.net/2248/1923
dc.description.abstract	Star 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.extent	269088 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/1999BASI...27..167K	en
dc.subject	Infrared emission	en
dc.subject	Star formation	en
dc.subject	Molecular cloud	en
dc.title	Infrared spectral energy distribution of four star forming regions	en
dc.type	Article	en