Transition probabilities have been derived for 20 5s-5p transitions of Pd I from a combination of radiative lifetime measurements for 6 odd-parity levels with time-resolved laser-induced fluorescence spectroscopy and of branching fraction determination using a hollow cathode discharge lamp. Additional oscillator strengths for 18 transitions have been determined from measured lifetimes and theoretical branching fractions obtained from configuration interaction calculations with core-polarization effects included. These new results have allowed us to refine the palladium abundance in the solar photosphere: APd = 1.66±0.04, in the usual logarithmic scale, a result in close agreement with the meteoritic value. © ESO 2006.
CITATION STYLE
Xu, H. L., Sun, Z. W., Dai, Z. W., Jiang, Z. K., Palmeri, P., Quinet, P., & Biémont, É. (2006). Radiative lifetimes, branching fractions and oscillator strengths in Pd i and the solar palladium abundance. Astronomy and Astrophysics, 452(1), 357–362. https://doi.org/10.1051/0004-6361:20054610
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