Strong, spatially extended CO 7 to 6 emission from luminous cloud cores: W51 and DR21

Details Strong, spatially extended CO 7 to 6 emission from luminous cloud cores: W51 and DR21 Strong, spatially extended CO 7 to 6 emission from luminous cloud cores: W51 and DR21

Oct 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988stin...8925106j&link_type=abstract

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Astronomy and Astrophysics

Astronomy

Carbon Monoxide, Mapping, Molecular Clouds, Nebulae, Absorption Spectra, Brightness Distribution, Galactic Nuclei, Galactic Radiation, Radio Sources (Astronomy)

Scientific paper

It is concluded that three distinct molecular cloud components contribute to the CO 7 vs 6 emission, including the warm, dynamically active material which accounts for 75 percent of the velocity integrated CO emission from the two sources; a warm, quiescent material associated with the HII regions in each source; and a cool (20 to 40K) quiescent gas, which overlies some of the hot material.

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