Transitions for FeIII (Quinet 1996)

Details Transitions for FeIII (Quinet 1996) Transitions for FeIII (Quinet 1996)

Nov 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995ycat..41160573q&link_type=abstract

VizieR On-line Data Catalog: J/A+AS/116/573. Originally published in: 1996A&AS..116..573Q

Physics

Atomic Physics

Atomic Physics

Scientific paper

Radiative transition probabilities have been calculated for states within the 3d6 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. (1 data file).

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