Collisional excitation of interstellar molecules - Linear molecules CO, CS, OCS, and HC3N

Details Collisional excitation of interstellar molecules - Linear molecules CO, CS, OCS, and HC3N Collisional excitation of interstellar molecules - Linear molecules CO, CS, OCS, and HC3N

Jun 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978apjs...37..169g&link_type=abstract

Astrophysical Journal Supplement Series, vol. 37, June 1978, p. 169-194.

Astronomy and Astrophysics

Astrophysics

285

Carbon Compounds, Cyanoacetylene, Interstellar Chemistry, Interstellar Gas, Molecular Collisions, Molecular Excitation, Abundance, Carbon Monoxide, Gas Temperature, Helium, Sulfur Compounds, Tables (Data)

Scientific paper

Rates for excitation of CO, CS, OCS, and HC3N by collisions with He atoms and H2 molecules are presented. These have been obtained from extensive theoretical calculations using methods of known reliability. In general, rates necessary for modeling interstellar molecular clouds with kinetic temperatures to 100 K have been included. Methods for fitting these rates in more compact form are discussed.

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