RADIATIVE CHARGE TRANSFER BETWEEN H AND $C^{++}, C^{+++}$ AND $N^{++}$

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1977

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Ohio State University

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Abstract

Radiative charge transfer with atomic hydrogen is described by: $$X^{+n} + H {\rightarrow} X^{+(n - 1)} + H^{+} + h _{\nu}.$$ In the present study, n=2,3 for $X = $C, and n=2 for $X = $N. Ab initioh calculations of the rate coefficients will be described. All molecular valence states in the exit channel which have a dipole allowed transition from the states of the entrance channel have been considered. The rate coefficients increase slowly with increasing temperature and attain values between 2×10−14 and 6×10−14 cm3 sec−1 at 104 K.

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This research was supported, in part, by the Energy Research and Development Administration under Contract EY-76-S-02-2887.


Author Institution: Center for Astrophysics, Harvard College Observatory, and Smithsonian Astrophysical Observatory

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