Radiative association in dense, H2-containing interstellar clouds

Astronomy and Astrophysics – Astrophysics

Scientific paper

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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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