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Stark Broadening in Compact Stars: Xe VI Lines

Authorized Users Only
2015
Authors
Dimitrijević, Milan S.
Simić, Zoran
Kovačević, Anđelka
Valjarević, Aleksandar
Sahal-Brechot, Sylvie
Conference object (Published version)
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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.
Keywords:
Stark broadening / atomic data / white dwarfs / Xe VI
Source:
Journal of Astrophysics and Astronomy, 2015, 36, 4, 681-691
Publisher:
  • Indian Acad Sciences, Bangalore
Funding / projects:
  • Influence of collisions on astrophysical plasma spectra (RS-176002)
  • Paris Observatory
  • Centre National de la Recherche Scientifique (CNRS) - European Commission
  • PNPS (Programme National de Physique Stellaire, INSU-CNRS)
  • Investissements d'avenir, French National Research Agency (ANR) [ANR-11-IDEX-0004-02]

DOI: 10.1007/s12036-015-9352-y

ISSN: 0250-6335

WoS: 000368698700023

Scopus: 2-s2.0-84956613605
[ Google Scholar ]
1
1
Handle
https://hdl.handle.net/21.15107/rcub_gery_728
URI
https://gery.gef.bg.ac.rs/handle/123456789/728
Collections
  • Radovi istraživača
Institution/Community
Geografski fakultet
TY  - CONF
AU  - Dimitrijević, Milan S.
AU  - Simić, Zoran
AU  - Kovačević, Anđelka
AU  - Valjarević, Aleksandar
AU  - Sahal-Brechot, Sylvie
PY  - 2015
UR  - https://gery.gef.bg.ac.rs/handle/123456789/728
AB  - 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.
PB  - Indian Acad Sciences, Bangalore
C3  - Journal of Astrophysics and Astronomy
T1  - Stark Broadening in Compact Stars: Xe VI Lines
VL  - 36
IS  - 4
SP  - 681
EP  - 691
DO  - 10.1007/s12036-015-9352-y
UR  - https://hdl.handle.net/21.15107/rcub_gery_728
ER  - 
@conference{
author = "Dimitrijević, Milan S. and Simić, Zoran and Kovačević, Anđelka and Valjarević, Aleksandar and Sahal-Brechot, Sylvie",
year = "2015",
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.",
publisher = "Indian Acad Sciences, Bangalore",
journal = "Journal of Astrophysics and Astronomy",
title = "Stark Broadening in Compact Stars: Xe VI Lines",
volume = "36",
number = "4",
pages = "681-691",
doi = "10.1007/s12036-015-9352-y",
url = "https://hdl.handle.net/21.15107/rcub_gery_728"
}
Dimitrijević, M. S., Simić, Z., Kovačević, A., Valjarević, A.,& Sahal-Brechot, S.. (2015). Stark Broadening in Compact Stars: Xe VI Lines. in Journal of Astrophysics and Astronomy
Indian Acad Sciences, Bangalore., 36(4), 681-691.
https://doi.org/10.1007/s12036-015-9352-y
https://hdl.handle.net/21.15107/rcub_gery_728
Dimitrijević MS, Simić Z, Kovačević A, Valjarević A, Sahal-Brechot S. Stark Broadening in Compact Stars: Xe VI Lines. in Journal of Astrophysics and Astronomy. 2015;36(4):681-691.
doi:10.1007/s12036-015-9352-y
https://hdl.handle.net/21.15107/rcub_gery_728 .
Dimitrijević, Milan S., Simić, Zoran, Kovačević, Anđelka, Valjarević, Aleksandar, Sahal-Brechot, Sylvie, "Stark Broadening in Compact Stars: Xe VI Lines" in Journal of Astrophysics and Astronomy, 36, no. 4 (2015):681-691,
https://doi.org/10.1007/s12036-015-9352-y .,
https://hdl.handle.net/21.15107/rcub_gery_728 .

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