Astronomy and Astrophysics – Astrophysics
Scientific paper
Oct 1981
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981apj...249..399w&link_type=abstract
Astrophysical Journal, Part 1, vol. 249, Oct. 1, 1981, p. 399-401.
Astronomy and Astrophysics
Astrophysics
84
Ion Recombination, Iron, Metal Ions, Photoionization, Radiative Recombination, Recombination Coefficient, Ion Production Rates, Ionization Cross Sections, Transition Probabilities
Scientific paper
Radiative recombination coefficients for all Fe ions are calculated by use of the Milne relation of detailed balance. Analytic fits are made to the dielectronic recombination rates computed by Jacobs (1977) and the Burgess general formula (1965). Higher level rates are treated hydrogenically by a quantum defect method based on the energies of the levels. Recombination coefficients for Fe I to Fe 26 are listed.
Sarazin Craig L.
Shull Michael J.
Woods Tod D.
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