Infrared emission from IRAS 00338+6312

dc.contributor.author	Mookerjea, B
dc.contributor.author	Ghosh, S. K
dc.contributor.author	Karnik, A. D
dc.contributor.author	Rengarajan, T. N
dc.contributor.author	Tandon, S. N
dc.contributor.author	Verma, R. P
dc.date.accessioned	2007-10-24T09:03:25Z
dc.date.available	2007-10-24T09:03:25Z
dc.date.issued	1999
dc.identifier.citation	BASI, Vol. 27, No. 1, pp. 155 - 158	en
dc.identifier.uri	http://hdl.handle.net/2248/1920
dc.description.abstract	The 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.extent	201211 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..155M	en
dc.subject	Infrared emission	en
dc.subject	IRAS 00338+6312	en
dc.subject	ZAMS star	en
dc.title	Infrared emission from IRAS 00338+6312	en
dc.type	Article	en