Stark Broadening in Compact Stars: Xe VI Lines

  • Milan S. Dimitrijević
  • Zoran Simić
  • Andjelka Kovačević
  • Aleksandar Valjarević
  • Sylvie Sahal-Bréchot
Review

DOI: 10.1007/s12036-015-9352-y

Cite this article as:
Dimitrijević, M.S., Simić, Z., Kovačević, A. et al. J Astrophys Astron (2015) 36: 0. doi:10.1007/s12036-015-9352-y
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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.

Key words

Stark broadening atomic data white dwarfs Xe VI. 

Copyright information

© Indian Academy of Sciences 2015

Authors and Affiliations

  • Milan S. Dimitrijević
    • 1
    • 2
    • 3
  • Zoran Simić
    • 1
  • Andjelka Kovačević
    • 4
  • Aleksandar Valjarević
    • 5
  • Sylvie Sahal-Bréchot
    • 2
  1. 1.Astronomical ObservatoryBelgradeSerbia
  2. 2.LERMA, Observatoire de Paris, PSL Research University, CNRSSorbonne Universities, UPMC Univ. Paris 06Meudon CedexFrance
  3. 3.IHIS Techno ExpertsBelgrade-ZemunSerbia
  4. 4.Department of AstronomyFaculty of MathematicsBelgradeSerbia
  5. 5.Faculty of Natural Sciences and Mathematics, Department of GeographyUniversity of Kosovska MitrovicaKosovska MitrovicaSerbia

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