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Title:
Recombination coefficients for iron ions [ Erratum: 1982ApJ...257..918W ]
Authors:
Woods, D. T.; Shull, J. M.; Sarazin, C. L.
Affiliation:
AA(Joint Institute for Laboratory Astrophysics; Colorado, University, Boulder, CO), AB(Joint Institute for Laboratory Astrophysics; Colorado, University, Boulder, CO), AC(Virginia, University; National Radio Astronomy Observatory, Charlottesville, VA)
Publication:
Astrophysical Journal, Part 1, vol. 249, Oct. 1, 1981, p. 399-401. (ApJ Homepage)
Publication Date:
10/1981
Category:
Atomic and Molecular Physics
Origin:
STI
NASA/STI Keywords:
Ion Recombination, Iron, Metal Ions, Photoionization, Radiative Recombination, Recombination Coefficient, Ion Production Rates, Ionization Cross Sections, Transition Probabilities
DOI:
10.1086/159298
Bibliographic Code:
1981ApJ...249..399W

Abstract

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.

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