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Lifetime measurements in Ru II and calculated oscillator strengths in Ru II and Ru III

P Palmeri1, P Quinet1,2, V Fivet1, É Biémont1,2, C R Cowley3, L Engström4, H Lundberg4, H Hartman5 and H Nilsson5

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A 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.


PACS

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)

Subjects

Atomic and molecular physics

Instrumentation and measurement

Dates

Issue 16 (28 August 2009)

Received 27 April 2009, in final form 18 June 2009

Published 22 July 2009



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