Radiative lifetimes of 22 levels in Rh I and of 35 levels in Ta I are reported. The lifetimes are measured with the use of time-resolved laser-induced fluorescence on an atomic beam. The Rh I lifetimes resolve the discrepancy between the spectroscopically determined solar abundance of Rh and the abundance of Rh determined from chondritic meteorites.
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Salih et al. (1983) studied this question.
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