Astronomy and Astrophysics – Astrophysics
Scientific paper
Sep 1979
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979a%26a....78..177m&link_type=abstract
Astronomy and Astrophysics, vol. 78, no. 2, Sept. 1979, p. 177-180.
Astronomy and Astrophysics
Astrophysics
18
Atomic Collisions, Charge Exchange, Hydrogen Atoms, Interstellar Gas, Ion Atom Interactions, Nitrogen, Astronomical Models, Graphs (Charts), Interstellar Matter, Ion Charge, Tables (Data)
Scientific paper
The cross section for the N(3 plus)-H charge exchange reaction is calculated within the framework of the molecular model of atomic collisions. The potential energy curves of the NH(3 plus) molecular ion are determined by a model potential method. The scattering equations describing the collision are derived in a fully quantal approach and solved to obtain the S-matrix. For temperatures less than 400 K, the reaction rate remains fairly constant of the order of 2-3 x 10 to the -10 cu cm/s (a minimum of 2 x 10 to the -10 cu cm/s occurs at 300 K). For temperatures exceeding 400 K the reaction rate increases with T, attaining 8 x 10 to the -9 cu cm/s at 30,000 K.
McCarroll R.
Valiron Pierre
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