Astronomy and Astrophysics – Astronomy
Scientific paper
Aug 1998
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998apj...502.1006s&link_type=abstract
Astrophysical Journal v.502, p.1006
Astronomy and Astrophysics
Astronomy
25
Atomic Processes, Ism: Atoms, Stars: Supernovae: Individual Alphanumeric: Sn 1987A
Scientific paper
Charge transfer rate coefficients for collisions of C+ with H and H+ with C are presented for temperatures from 30,000 to 107 K and from 10 to 107 K, respectively. The rate coefficients were calculated from recommended cross sections deduced in a recent theoretical and experimental investigation that took into account previous measurements. Nonadiabatic radial coupling is the dominant mechanism for both reactions above ~50,000 K, but for lower temperatures the reaction of H+ with C proceeds primarily by radiative charge transfer. Implications, due to the magnitude of the rate coefficients, for various astrophysical environments are discussed.
Buenker Robert J.
Gu J. P.
Havener C. C.
Hirsch G.
Kimura Masahiro
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