Transition probabilities for forbidden lines of Fe III.

Details Transition probabilities for forbidden lines of Fe III. Transition probabilities for forbidden lines of Fe III.

May 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996a%26as..116..573q&link_type=abstract

Astronomy and Astrophysics Supplement, v.116, p.573-578

Astronomy and Astrophysics

Astrophysics

38

Atomic Data, Fe Iii, Radiative Transition Probabilities

Scientific paper

Radiative transition probabilities have been calculated for states within the 3d^6^ configuration of Fe III. 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. 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. The present work represents a refinement of previous monoconfigurational calculations of transition probabilities for forbidden lines of astrophysical interest in Fe III.

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