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      Permanent link:
      https://www.ias.ac.in/article/fulltext/joaa/036/04/0681-0691

    • Keywords

       

      Stark broadening; atomic data; white dwarfs; Xe VI.

    • 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.

    • Author Affiliations

       

      Milan S. Dimitrijević1 2 3 Zoran Simić1 Andjelka Kovačević4 Aleksandar Valjarević5 Sylvie Sahal-Bréchot2

      1. Astronomical Observatory, Volgina 7, 11060 Belgrade, Serbia.
      2. LERMA, Observatoire de Paris, PSL Research University, CNRS, Sorbonne Universities, UPMC Univ. Paris 06, 5 Place Jules Janssen, 92195 Meudon Cedex, France.
      3. IHIS Techno Experts, Bežanijski put 23, 11080 Belgrade-Zemun, Serbia.
      4. Department of Astronomy, Faculty of Mathematics, Studentski Trg 16, 11000 Belgrade, Serbia.
      5. Faculty of Natural Sciences and Mathematics, Department of Geography, University of Kosovska Mitrovica, Ive Lole Ribara 29, 38220 Kosovska Mitrovica, Serbia.
    • Dates

       
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