Oscillator strengths are given for transitions belonging to thea5S-z5P0anda5D-z5P0multiplets in Mn II. The data originate from beam-foil measurements of thez5P1,2,30level lifetimes and branching-ratio determinations. Theoreticalf-values are also given for these transitions, the agreement between experiment and theory being satisfactory. Using the experimentalgf-values obtained in this work and empirical solar models, the solar abundance of Mn has been determined to be logNMn= 5.4 ± 0.2 (on the logNH= 12.00 scale).
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Martinson et al. (1977) studied this question.
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