Inner-shell photoexcitation of FeXV and FeXVI

Details Inner-shell photoexcitation of FeXV and FeXVI Inner-shell photoexcitation of FeXV and FeXVI

Sep 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003mnras.344..696k&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Volume 344, Issue 3, pp. 696-706.

Astronomy and Astrophysics

Astronomy

1

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

Scientific paper

The configuration-interaction method as implemented in the computer code CIV3 is used to determine energy levels, electric dipole radiative transition wavelengths, oscillator strengths and transition probabilities for inner-shell excitation of transitions in FeXV and FeXVI. Specifically, transitions are considered of the type 1s22s22p63s2-1s22s22p53l3l'3l'' (l, l' and l''= s, p or d) in FeXV and 1s22s22p63s-1s22s22p53l3l' (l and l'= s, p or d) in FeXVI, using the relativistic Breit-Pauli approach. An assessment of the accuracy of the derived atomic data is performed.

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