Cross sections and rate coefficients for total and fine-structure resolved charge transfer in collisions of O+ with H and H+ with O are presented for collision energies between 0.1 meV/u and 10 MeV/u and temperatures between 10 and 107 K. The results are obtained utilizing new quantal and semiclassical molecular-orbital close-coupling, classical trajectory Monte Carlo, and continuum distorted wave calculations in conjunction with previous experimental and theoretical data. Applications to various astrophysical and atmospheric environments are discussed.
CITATION STYLE
Stancil, P. C., Schultz, D. R., Kimura, M., Gu, J. P., Hirsch, G., & Buenker, R. J. (1999). Charge transfer in collisions of O+ with H and H+ with O. Astronomy and Astrophysics Supplement Series, 140(2), 225–234. https://doi.org/10.1051/aas:1999419
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