Stark Broadening in Compact Stars: Xe VI LinesReportar como inadecuado

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* Corresponding author 1 LERMA - Laboratoire d-Etude du Rayonnement et de la Matière en Astrophysique 2 Astronomical Observatory 3 Department of Astronomy 4 Department of Geography

Abstract : 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.

Keywords : Stark broadening atomic data white dwarfs Xe VI.

Autor: Milan S. Dimitrijević - Zoran Simić - Andjelka Kovačević - Aleksandar Valjarević - Sylvie Sahal-Bréchot -



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