Radiative association in dense, H2-containing interstellar clouds

Details Radiative association in dense, H2-containing interstellar clouds Radiative association in dense, H2-containing interstellar clouds

Apr 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976apj...205...94h&link_type=abstract

Astrophysical Journal, vol. 205, Apr. 1, 1976, pt. 1, p. 94-102.

Astronomy and Astrophysics

Astrophysics

42

Chemical Reactions, Hydrogen Clouds, Interstellar Gas, Molecular Collisions, Reaction Kinetics, Abundance, Amines, Imines, Methyl Compounds, Molecular Ions, Polyatomic Molecules

Scientific paper

A method for estimating the order of magnitude of rate coefficients of radiative-association reactions involving polyatomic species is outlined. Calculations are undertaken on reactions of possible importance in dense interstellar clouds. Several of the calculated rate coefficients are utilized in a study of the gas-phase syntheses of H2CNH (methanimine) and H3CNH2 (methylamine).

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