Far-infrared observations of three galactic star-forming regions: RCW 36, IRAS 10361-5830 and IRAS 10365-5803

Details Far-infrared observations of three galactic star-forming regions: RCW 36, IRAS 10361-5830 and IRAS 10365-5803 Far-infrared observations of three galactic star-forming regions: RCW 36, IRAS 10361-5830 and IRAS 10365-5803

Apr 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994a%26a...284..936v&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 284, no. 3, p. 936-948

Astronomy and Astrophysics

Astronomy

10

Astronomical Maps, Far Infrared Radiation, H Ii Regions, Infrared Astronomy, Interstellar Matter, Milky Way Galaxy, Star Formation, Balloon-Borne Instruments, Bolometers, Fir Filters, Photometers, Space Temperature, Stellar Luminosity, Telescopes

Scientific paper

Three Southern star-forming regions -- RCW 36, IRAS 10361-5830 and IRAS 10365-5803, have been observed simultaneously in two far-infrared bands with effective wavelengths of 58 micrometers and 150 micrometers using the Tata Institute of Fundamental Research (TIFR) 100 cm balloon-borne telescope. Intensity maps of these sources have been obtained covering areas of approximately 15 min x 20 min around each source, with an angular resolution of approximately 1.5 min. Multiple sources have been detected in each map. Luminosities and dust temperatures for individual sources have been derived. Data from IRAS Pointed Observations at 12, 25, 60 and 100 micrometers have been deconvolved to generate high resolution maps of these regions and these have been compared with our maps.

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