Carbon monoxide mapping of 100 micrometer sources associated with dark clouds: Preliminary results

Details Carbon monoxide mapping of 100 micrometer sources associated with dark clouds: Preliminary results Carbon monoxide mapping of 100 micrometer sources associated with dark clouds: Preliminary results

Nov 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974hrgc.conf..203s&link_type=abstract

H II regions and the galactic centre : proceedings of the Eighth ESLAB Symposium, 4-7 June 1974, Frascati, Italy, p. 203-207 (SE

Astronomy and Astrophysics

Astronomy

2

Carbon Monoxide, Galactic Radiation, Hydrogen Clouds, Mapping, Radiation Sources, Astronomical Maps, Cosmic Dust, Far Infrared Radiation, Submillimeter Waves

Scientific paper

Since molecules seem to be associated with regions of dust and gas, a program was initiated of CO mapping observations of 100 microns sources that were detected in the several airborne surveys in order to study the temperature, optical depth, and excitation conditions in these sources. The first sources to be mapped were HFE 2, 9, 10, and 11 and FJM 3. CO was found at or near all the 100 microns sources (with the exception of HFE 10 and 11), and the sources appear to be associated with small dark clouds.

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