Breit-Pauli energy levels, transition probabilities and lifetimes for 3d5 levels in FeIV of astrophysical interest

Details Breit-Pauli energy levels, transition probabilities and lifetimes for 3d5 levels in FeIV of astrophysical interest Breit-Pauli energy levels, transition probabilities and lifetimes for 3d5 levels in FeIV of astrophysical interest

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004mnras.355..461f&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Volume 355, Issue 2, pp. 461-474.

Astronomy and Astrophysics

Astronomy

10

Atomic Data, Atomic Processes

Scientific paper

Energy levels, lifetimes and transition probabilities for transitions between computed levels of 3d5 of FeIV are reported. The E2 and M1 transition probabilities are compared with earlier theoretical results, often only the values published by Garstang in 1958. From the available astronomical observations of optical emission lines arising from the same level, a few direct tests are now possible and they show consistency with the theoretical calculations.

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