Abstract

Branching ratios and absolute transition probabilities for 115 lines in rhodium i are reported. The branching ratios generally agree with branching ratios deduced from the Corliss–Bozman monograph. Although there are some revisions of branching ratios used in recent work on the solar abundance of Rh, the scatter in solar-abundance values determined from different lines is not reduced by the revised branching ratios.

© 1985 Optical Society of America

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