Astronomy and Astrophysics – Astrophysics
Scientific paper
Dec 1999
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999a%26as..140..225s&link_type=abstract
Astronomy and Astrophysics Supplement, v.140, p.225-234
Astronomy and Astrophysics
Astrophysics
46
Atomic Processes, Ism: Atoms, Interplanetary Medium, Comets: General, Planets And Satellites: Individual: Jupiter
Scientific paper
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.
Buenker Robert J.
Gu J. P.
Hirsch G.
Kimura Masahiro
Schultz David R.
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