Theoretical calculation for the hyperfine collisional transition rate coefficients of interstellar type-A CH3CN-H2.

Details Theoretical calculation for the hyperfine collisional transition rate coefficients of interstellar type-A CH3CN-H2. Theoretical calculation for the hyperfine collisional transition rate coefficients of interstellar type-A CH3CN-H2.

Mar 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995acasn..36....7p&link_type=abstract

Acta Astron. Sin., Vol. 36, No. 1, p. 7 - 20

Astronomy and Astrophysics

Astronomy

Interstellar Molecules: Transition Probabilities

Scientific paper

Using IOS (infinite order sudden) approximation, the hyperfine collisional transition rate coefficients of type-A CH3CN-H2 are calculated under the conditions of interstellar molecular clouds. The range of kinetic temperature is between 20 and 140K. The results provide useful fundamental molecular data for studying physical and chemical properties of molecular cloud and star forming region.

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