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Computation of oscillator strengths by a semiempirical method for some elements of the iron group and their solar photospheric abundance

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Abstract

Absolute oscillator strengths are computed by the STF method for selected lines of Sci.The lifetimes deduced from these values are in satisfactory agreement with recent beam-foil measurements. From a study of 10 selected lines, a new value of the solar photospheric abundance is derived (logN sc = 3.04) in agreement with the meteoritic value.

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  1. Institut d'Astrophysique, Université de Liège, 4200, Cointe-Ougrée, Belgique

    E. Biémont

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  1. E. Biémont
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Biémont, E. Computation of oscillator strengths by a semiempirical method for some elements of the iron group and their solar photospheric abundance. Sol Phys 39, 305–308 (1974). https://doi.org/10.1007/BF00162422

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  • DOI: https://doi.org/10.1007/BF00162422

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