Astronomy and Astrophysics – Astrophysics
Scientific paper
Jan 2001
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001a%26a...365..266t&link_type=abstract
Astronomy and Astrophysics, v.365, p.266-267 (2001)
Astronomy and Astrophysics
Astrophysics
1
Atomic Data
Scientific paper
We tabulate theoretical line strengths, f-values and transition energies for the beryllium-like ion Fe xxiii. Transitions are between levels 2l_1 2l_2 S'L'J' and 2l_3 nl_4 SLJ with n = 2, 3, 4. The calculation uses the well known configuration interaction program CIV3 in which relativistic effects are allowed for by means of the Breit-Pauli approximation. We give a detailed comparison of our oscillator strengths with those which Chen & Ong (\cite{Chen98}) obtained using the relativistic Dirac code GRASP2. Tables 1 to 17 are only available in electronic form at http://www.edpsciences.org
Chidichimo Marita C.
Tully John A.
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