Astronomy and Astrophysics – Astrophysics
Scientific paper
Jun 1995
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995a%26as..111..333b&link_type=abstract
Astronomy and Astrophysics Supplement, v.111, p.333
Astronomy and Astrophysics
Astrophysics
24
Atomic Data, 5P^K^, Radiative Transition Probabilities
Scientific paper
Energy levels and radiative transition probabilities have been calculated for states within the 5p^k^ (k =1-5) configurations of atoms and ions in the indium, tin, antimony, tellurium and iodine isoelectronic sequences up to cerium. Magnetic dipole (M1) and electric quadrupole (E2) transition probabilities have been obtained using average energies, electrostatic and spin-orbit integrals adjusted so as to fit the observed energy levels or in the absence of experimental data by graphical extrapolation along the sequences. The most important configuration interaction (CI) and relativistic effects were included explicitly in the calculations, using the relativistic Hartree-Fock (HFR) method due to Cowan. For many of the forbidden lines of astrophysical interest considered in the present work, transition probabilities are reported for the first time.
Biémont É.
Hansen James E.
Quinet Pascal
Zeippen Claude J.
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