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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:E. Biémont
Affiliation:(1) Institut d'Astrophysique, Université de Liège, B-4200 Cointe-Ougrée, Belgium
Abstract:Oscillator strengths calculated by the STF method for selected transitions of V i and Co i have permitted to deduce, from an LTE study of weak lines, photospheric abundances in agreement with those obtained from carbonaceous chondrites. A summary of results is also presented for all the iron-group elements.
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