Stark Broadening in Compact Stars: Xe VI Lines
Milan S. Dimitrijević Zoran Simić Andjelka Kovačević Aleksandar Valjarević Sylvie Sahal-Bréchot
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We will consider Stark broadening of non hydrogenic spectral lines in the impact approximation in compact stars: pre-white dwarf and white dwarf atmospheres. In order to show an example, Stark broadening parameters have been calculated, using the impact semiclassical perturbation approach for four Xe VI spectral lines. Obtained results have been used to demonstrate the influence of Stark broadening in DA and DB white dwarf atmospheres.
Milan S. Dimitrijević1 2 3 Zoran Simić1 Andjelka Kovačević4 Aleksandar Valjarević5 Sylvie Sahal-Bréchot2
Volume 41, 2020
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