Balloon-borne far-infrared mapping of galactic star forming regions

Das, B. ; Ghosh, S. K. ; Rengarajan, T. N. ; Verma, R. P. ; Iyengar, K. V. K. ; Tandon, S. N. (1993) Balloon-borne far-infrared mapping of galactic star forming regions Bulletin of the Astronomical Society of India, 21 (3-4). pp. 587-590. ISSN 0304-9523

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Official URL: http://adsabs.harvard.edu/abs/1993BASI...21..587D

Abstract

Large angular areas (greater than 500 sq arcmin each) covering the three Galactic star forming regions (NGC 2024, OMC-1/OMC-2, and IRAS 06058+2138 and its neighborhood) have been mapped in two FIR bands (58 and 150 micrometers) with approximately 1.5 arcmin resolution using the Tata Institute of Fundamental Research (TIFR) 100 cm balloon-borne telescope. The resulting intensity maps as well as color temperature and optical depth (for NGC 2024 only) maps are presented and their implications are discussed.

Item Type:Article
Source:Copyright of this article belongs to Astronomical Society of India.
Keywords:Infrared Imagery; Interstellar Gas; Milky Way Galaxy; Molecular Clouds; Star Formation; Stellar Spectrophotometry; Balloon-borne Instruments; Image Analysis; Luminosity; Radio Spectra; Spectrum Analysis; Telescopes
ID Code:51679
Deposited On:29 Jul 2011 06:07
Last Modified:15 Jul 2012 10:55

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