Inner-shell photoexcitation of Fe XV and Fe XVI
Kisielius R., Hibbert A., Ferland G.J., Foord M.E., Rose S.J., van Hoof P.A.M., Keenan F.P.
published in: MNRAS, 344, 696 (2003)
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 Fe XV and Fe XVI. Specifically, transitions are considered of the type
1s22s22p63s2 -
1s22s22p53l3l'3l'' (l, l' and l'' = s, p or d)
in Fe XV and 1s22s22p63s -
1s22s22p53l3l' (l and l' = s, p or d) in Fe XVI,
using the relativistic Breit-Pauli approach. An assessment of the accuracy of the
derived atomic data is performed.
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Peter van Hoof
Royal Observatory of Belgium
Ringlaan 3
1180 Brussel
Belgium
email: p DOT vanhoof AT oma DOT be
