TY - JOUR
T1 - Inner-shell photoexcitation of Fe XV and Fe XVI
AU - Kisielius, R.
AU - Hibbert, A.
AU - Ferland, G. J.
AU - Foord, M. E.
AU - Rose, S. J.
AU - Van Hoof, P. A.M.
AU - Keenan, F. P.
PY - 2003/9/21
Y1 - 2003/9/21
N2 - 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 1s22s22p63s 2-1s22s22p53l3l′3lPrime; (l, l′ and l″ = s, p or d) in Fe xv and 1s22s 22p63s-1s22s22p 53l3l′ (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.
AB - 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 1s22s22p63s 2-1s22s22p53l3l′3lPrime; (l, l′ and l″ = s, p or d) in Fe xv and 1s22s 22p63s-1s22s22p 53l3l′ (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.
KW - Atomic data
KW - Line: formation
KW - X-rays: general
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U2 - 10.1046/j.1365-8711.2003.06801.x
DO - 10.1046/j.1365-8711.2003.06801.x
M3 - Article
AN - SCOPUS:0142260959
SN - 0035-8711
VL - 344
SP - 696
EP - 706
JO - Monthly Notices of the Royal Astronomical Society
JF - Monthly Notices of the Royal Astronomical Society
IS - 3
ER -