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Computation of oscillator strengths by a semi-empirical method for some elements of the iron-group and their solar photospheric abundance
Authors:Emile Biemont
Institution:1. Institut d'Astrophysique, Université de Liège, B-4200, Cointe-Ougrée, Belgique
Abstract:Oscillator strengths are calculated by the STF method for selected transitions of Mn i. The results, applied to the analysis of solar spectra, support the ‘high’ solar photospheric abundance of manganese recently obtained on the basis of experimental gf-values.
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