Infrared spectroscopic diagnostics for initial mass function

dc.contributor.author	Ghosh, S. K
dc.contributor.author	Mookerjea, B
dc.date.accessioned	2007-10-24T07:40:24Z
dc.date.available	2007-10-24T07:40:24Z
dc.date.issued	1999
dc.identifier.citation	BASI, Vol. 27, No. 1, pp. 151 - 154	en
dc.identifier.uri	http://hdl.handle.net/2248/1919
dc.description.abstract	The diagnostic values of various atomic/ nebular infrared spectral lines of relatively abundant elements (in different ionization states) in Galactic star forming regions, have been studied quantitatively. The code CLOUDY (Ferland 1996)has been used to model spherically symmetric interstellar clouds with embedded ZAMS stars / Young star clusters. In particular, the question of deciphering the upper mass limit of initial mass function has been addressed, in the light of the capabilities of the two spectrometers onboard Infrared Space Observatory (ISO-SWS covering 2.5 - 45 μm; & ISO-LWS covering 45 - 200 μm).	en
dc.format.extent	261688 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..151G	en
dc.subject	Infrared Spectral lines	en
dc.subject	Spectroscopic	en
dc.subject	Mass function	en
dc.subject	Infrared space observatory(ISO)	en
dc.title	Infrared spectroscopic diagnostics for initial mass function	en
dc.type	Article	en