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Stark Broadening Data for Stellar Plasma Research

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Abstract

Results of an effort to provide to astrophysicists and physicists a set of Stark broadening parameters that is as complete as possible are presented. Such parameters are needed for stellar opacity calculations, stellar atmosphere modelling, abundance determinations, and diagnostics of various plasmas in astrophysics, physics, and plasma technology. The Stark broadening was treated using a semiclassical perturbation and modified semiempirical approaches.

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Authors and Affiliations

  1. Astronomical Observatory, Volgina 7, 11050 Belgrade, Serbia, Yugoslavia

    Milan S. Dimitrijević

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  1. Milan S. Dimitrijević
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Dimitrijević, M.S. Stark Broadening Data for Stellar Plasma Research. Astrophysics and Space Science 252, 415–422 (1997). https://doi.org/10.1023/A:1000825624479

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