Radiative Recombination Rate Coefficients for Bare through F-like Isosequences of Mg, Si, S, Ar, Ca, Fe, and Ni

Details Radiative Recombination Rate Coefficients for Bare through F-like Isosequences of Mg, Si, S, Ar, Ca, Fe, and Ni Radiative Recombination Rate Coefficients for Bare through F-like Isosequences of Mg, Si, S, Ar, Ca, Fe, and Ni

Jun 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003apj...589.1085g&link_type=abstract

The Astrophysical Journal, Volume 589, Issue 2, pp. 1085-1088.

Astronomy and Astrophysics

Astronomy

39

Atomic Data, Atomic Processes

Scientific paper

We present distorted-wave calculations and analytic fits to the radiative recombination rate coefficients of bare to F-like isosequences of seven abundant astrophysical elements, including Mg, Si, S, Ar, Ca, Fe, and Ni. The fits are valid over a wide range of temperature, from 10-4 to 104 eV. Extensive comparisons with existing data are made.

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