Energetic N(+) ions in the interstellar medium

Details Energetic N(+) ions in the interstellar medium Energetic N(+) ions in the interstellar medium

Jul 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987mnras.227..461y&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 227, July 15, 1987, p. 461-466.

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17

Computational Chemistry, Energetic Particles, Gas-Ion Interactions, Interstellar Chemistry, Molecular Clouds, Nitrogen Ions, Computational Astrophysics, Gas Temperature, Reaction Kinetics

Scientific paper

Energetic N+ ions are produced in interstellar clouds by reactions of He+ ions and N2 with sufficient energy to overcome the exoergicity of the reaction of N+ with H2 and thereby from NH+ ions. The reacting N+ ions also slow down by elastic collisions with the ambient H2 molecules. The equilibrium energy distributions of the N+ ions in a gas with temperature between 10 and 70K are derived and the effective reaction rate coefficients are calculated. At 30K, the rate coefficient is 1.6×10-10cm3s-1.

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