Theoretical calculation for the collisional transitional rate coefficients of interstellar E-type CH3CN-H2.

Details Theoretical calculation for the collisional transitional rate coefficients of interstellar E-type CH3CN-H2. Theoretical calculation for the collisional transitional rate coefficients of interstellar E-type CH3CN-H2.

Jun 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995acasn..36..213p&link_type=abstract

Acta Astron. Sin., Vol. 36, No. 2, p. 213 - 215

Astronomy and Astrophysics

Astronomy

3

Interstellar Molecules: Transition Probabilities, Star-Forming Regions: Molecular Processes

Scientific paper

The collisional transitional rate coefficients of E-type
CH3CN-H2 are calculated under the conditions of
interstellar molecular clouds, which presents many fundamental data for
studying physical and chemical properties of molecular clouds and star
forming regions.

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