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Stark Broadening in Compact Stars: Xe VI Lines
Authors:Milan S Dimitrijevi?  Zoran Simi?  Andjelka Kova?evi?  Aleksandar Valjarevi?  Sylvie Sahal-Bréchot
Institution:1.Astronomical Observatory,Belgrade,Serbia;2.LERMA, Observatoire de Paris, PSL Research University, CNRS,Sorbonne Universities, UPMC Univ. Paris 06,Meudon Cedex,France;3.IHIS Techno Experts,Belgrade-Zemun,Serbia;4.Department of Astronomy,Faculty of Mathematics,Belgrade,Serbia;5.Faculty of Natural Sciences and Mathematics, Department of Geography,University of Kosovska Mitrovica,Kosovska Mitrovica,Serbia
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:
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