Radiative and Auger Decay of K-Vacancy Levels in the Ne, Mg, Si, S, Ar, and Ca Isonuclear Sequences

Details Radiative and Auger Decay of K-Vacancy Levels in the Ne, Mg, Si, S, Ar, and Ca Isonuclear Sequences Radiative and Auger Decay of K-Vacancy Levels in the Ne, Mg, Si, S, Ar, and Ca Isonuclear Sequences

Jul 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008apjs..177..408p&link_type=abstract

The Astrophysical Journal Supplement Series, Volume 177, Issue 1, pp. 408-416.

Astronomy and Astrophysics

Astronomy

17

Atomic Processes, Atomic Data, Line: Formation, X-Rays: General

Scientific paper

The HFR and AUTOSTRUCTURE atomic structure codes are used to compute complete data sets of level energies, wavelengths, A-values, and radiative and Auger widths for K-vacancy states of the Ne, Mg, Si, S, Ar, and Ca isonuclear sequences. Ions with electron number N>9 are treated for the first time. Detailed comparisons with previous measurements and theoretical data for ions with N<=9 are carried out in order to estimate reliable accuracy ratings.

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