CAOSP abstracts, Volume: 52, No.: 3, year: 2022

Abstract: Stark broadening parameters for four Sn III spectral line obtained by using semiclassical perturbation approach and Stark widths for this transitions obtained by using modified semiempirical approach have been compared with available experimental and semiempirical data and used for the consideration of the influence of the Stark broadening effect in A type stellar atmospheres.

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Last update: November 16, 2022