Study of carbon monoxide formation in interstellar clouds

Details Study of carbon monoxide formation in interstellar clouds Study of carbon monoxide formation in interstellar clouds

Jan 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985afz....22..163a&link_type=abstract

(Astrofizika, vol. 22, Jan.-Feb. 1985, p. 163-176) Astrophysics (ISSN 0571-7132), vol. 21, no. 1, July 1985, p. 100-107. Transla

Astronomy and Astrophysics

Astrophysics

1

Abundance, Atom Concentration, Carbon Monoxide, Interstellar Chemistry, Interstellar Gas, Molecular Clouds, Carbon, Gas Density, Gas Temperature, Heat Balance, Neutral Gases, Optical Thickness, Reaction Kinetics

Scientific paper

The concentrations of atoms and molecules, important for the thermal balance of interstellar clouds, are calculated as functions of the optical thickness for densities of 10 to 10,000 per cu cm and temperatures from 10 to 100 K. Emphasis is on the change in the concentrations of singly ionized carbon, C, and CO. The results can be used to construct models of interstellar clouds and calculate the intensities and profiles of the resulting radio lines.

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