P Palmeri et al 2009 J. Phys. B: At. Mol. Opt. Phys. 42 165005 doi:10.1088/0953-4075/42/16/165005
P Palmeri1, P Quinet1,2, V Fivet1, É Biémont1,2, C R Cowley3, L Engström4, H Lundberg4, H Hartman5 and H Nilsson5
Show affiliationsA new set of theoretical f-values is reported for 178 Ru II transitions of astrophysical interest, involving energy levels below 58 000 cm−1. The theoretical model, including core-polarization effects, has been tested by comparing theoretical lifetimes with new measurements performed by time-resolved laser-induced fluorescence spectroscopy for 23 4d6(5D)5p odd levels of Ru II and by comparing theoretical and experimental Landé g-factors. The first set of transition probabilities is proposed for 25 strong lines depopulating the 4d55p5,7P° terms of Ru III. The new results will allow quantitative investigations of stellar spectra and allow the astrophysicists to refine the ruthenium abundance in stars.
32.70.Cs Oscillator strengths, lifetimes, transition moments
07.57.-c Infrared, submillimeter wave, microwave and radiowave instruments and equipment
33.50.Dq Fluorescence and phosphorescence spectra
32.50.+d Fluorescence, phosphorescence (including quenching)
Issue 16 (28 August 2009)
Received 27 April 2009, in final form 18 June 2009
Published 22 July 2009
P Palmeri et al 2009 J. Phys. B: At. Mol. Opt. Phys. 42 165005
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