IRAS sources beyond the solar circle. I - CO observations

Details IRAS sources beyond the solar circle. I - CO observations IRAS sources beyond the solar circle. I - CO observations

Oct 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989a%26as...80..149w&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 80, no. 2, Oct. 1989, p. 149-187.

Astronomy and Astrophysics

Astrophysics

245

Carbon Monoxide, Infrared Astronomy Satellite, Molecular Clouds, Star Formation, Stellar Color, Stellar Luminosity, Bolometers, Galactic Nuclei, H Ii Regions, Missing Mass (Astrophysics), Telescopes, Water Masers

Scientific paper

C-12O (J = 1-0) has been observed with the 15-m SEST and the 30-m IRAM telescope in the direction of 1302 IRAS sources with colors of star forming regions located within 10 deg of the galactic plane in the interval between 85 and 280 deg. Emission components with line profiles that are non-Gaussian (showing, e.g., possible self-absorption or wings) are identified; this information may serve as a basis for selecting sources for future research. For all components, kinematic heliocentric and galactocentric distances, and distances from the galactic plane are derived. For those components which may be associated with the IRAS sources, bolometric luminosities are derived. These data will be analyzed and compared with HI data in subsequent papers.

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