TY  - JOUR
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/123456789/729
AB  - Stark broadening parameters have been calculated for 60 spectral lines of Xe VIII, for broadening by electron, proton, and He III impacts. For calculations, the semiclassical perturbation approach in the impact approximation has been used. The widths and shifts are provided for temperatures from 20 000 K to 500 000 K and for an electron density of 10(17) cm(-3). Obtained results have been used to study the influence of Stark broadening on spectral lines in DO white dwarf atmospheres and it has been found that exist broad layers where this broadening mechanism is dominant in comparison with thermal Doppler broadening.
PB  - Oxford Univ Press, Oxford
T2  - Monthly Notices of the Royal Astronomical Society
T1  - Stark broadening of Xe VIII spectral lines
VL  - 454
IS  - 2
SP  - 1736
EP  - 1741
DO  - 10.1093/mnras/stv1970
UR  - https://hdl.handle.net/21.15107/rcub_gery_729
ER  - 

@article{
author = "Dimitrijević, Milan S. and Simić, Zoran and Kovačević, Anđelka and Valjarević, Aleksandar and Sahal-Brechot, Sylvie",
year = "2015",
abstract = "Stark broadening parameters have been calculated for 60 spectral lines of Xe VIII, for broadening by electron, proton, and He III impacts. For calculations, the semiclassical perturbation approach in the impact approximation has been used. The widths and shifts are provided for temperatures from 20 000 K to 500 000 K and for an electron density of 10(17) cm(-3). Obtained results have been used to study the influence of Stark broadening on spectral lines in DO white dwarf atmospheres and it has been found that exist broad layers where this broadening mechanism is dominant in comparison with thermal Doppler broadening.",
publisher = "Oxford Univ Press, Oxford",
journal = "Monthly Notices of the Royal Astronomical Society",
title = "Stark broadening of Xe VIII spectral lines",
volume = "454",
number = "2",
pages = "1736-1741",
doi = "10.1093/mnras/stv1970",
url = "https://hdl.handle.net/21.15107/rcub_gery_729"
}

Dimitrijević, M. S., Simić, Z., Kovačević, A., Valjarević, A.,& Sahal-Brechot, S.. (2015). Stark broadening of Xe VIII spectral lines. in Monthly Notices of the Royal Astronomical Society
Oxford Univ Press, Oxford., 454(2), 1736-1741.
https://doi.org/10.1093/mnras/stv1970
https://hdl.handle.net/21.15107/rcub_gery_729

Dimitrijević MS, Simić Z, Kovačević A, Valjarević A, Sahal-Brechot S. Stark broadening of Xe VIII spectral lines. in Monthly Notices of the Royal Astronomical Society. 2015;454(2):1736-1741.
doi:10.1093/mnras/stv1970
https://hdl.handle.net/21.15107/rcub_gery_729 .

Dimitrijević, Milan S., Simić, Zoran, Kovačević, Anđelka, Valjarević, Aleksandar, Sahal-Brechot, Sylvie, "Stark broadening of Xe VIII spectral lines" in Monthly Notices of the Royal Astronomical Society, 454, no. 2 (2015):1736-1741,
https://doi.org/10.1093/mnras/stv1970 .,
https://hdl.handle.net/21.15107/rcub_gery_729 .

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 .

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/123456789/726
AB  - In order to complete Stark broadening data for Ne I spectral lines which are needed for analysis of stellar atmospheres, collisional widths and shifts (the so-called Stark broadening parameters) of 29 isolated spectral lines of neutral neon have been determined within the impact semiclassical perturbation method. Calculations have been performed for the broadening by collisions with electrons, protons and ionized helium for astrophysical applications, and for collisions with ionized neon and argon for laboratory plasma diagnostics. The shifts have been compared with existing experimental values. The obtained data will be included in the STARK-B database, which is a part of the Virtual Atomic and Molecular Data Center - VAMDC.
PB  - Indian Acad Sciences, Bangalore
C3  - Journal of Astrophysics and Astronomy
T1  - Stark Widths of Spectral Lines of Neutral Neon
VL  - 36
IS  - 4
SP  - 643
EP  - 659
DO  - 10.1007/s12036-015-9343-z
UR  - https://hdl.handle.net/21.15107/rcub_gery_726
ER  - 

@conference{
author = "Dimitrijević, Milan S. and Simić, Zoran and Kovačević, Anđelka and Valjarević, Aleksandar and Sahal-Brechot, Sylvie",
year = "2015",
abstract = "In order to complete Stark broadening data for Ne I spectral lines which are needed for analysis of stellar atmospheres, collisional widths and shifts (the so-called Stark broadening parameters) of 29 isolated spectral lines of neutral neon have been determined within the impact semiclassical perturbation method. Calculations have been performed for the broadening by collisions with electrons, protons and ionized helium for astrophysical applications, and for collisions with ionized neon and argon for laboratory plasma diagnostics. The shifts have been compared with existing experimental values. The obtained data will be included in the STARK-B database, which is a part of the Virtual Atomic and Molecular Data Center - VAMDC.",
publisher = "Indian Acad Sciences, Bangalore",
journal = "Journal of Astrophysics and Astronomy",
title = "Stark Widths of Spectral Lines of Neutral Neon",
volume = "36",
number = "4",
pages = "643-659",
doi = "10.1007/s12036-015-9343-z",
url = "https://hdl.handle.net/21.15107/rcub_gery_726"
}

Dimitrijević, M. S., Simić, Z., Kovačević, A., Valjarević, A.,& Sahal-Brechot, S.. (2015). Stark Widths of Spectral Lines of Neutral Neon. in Journal of Astrophysics and Astronomy
Indian Acad Sciences, Bangalore., 36(4), 643-659.
https://doi.org/10.1007/s12036-015-9343-z
https://hdl.handle.net/21.15107/rcub_gery_726

Dimitrijević MS, Simić Z, Kovačević A, Valjarević A, Sahal-Brechot S. Stark Widths of Spectral Lines of Neutral Neon. in Journal of Astrophysics and Astronomy. 2015;36(4):643-659.
doi:10.1007/s12036-015-9343-z
https://hdl.handle.net/21.15107/rcub_gery_726 .

Dimitrijević, Milan S., Simić, Zoran, Kovačević, Anđelka, Valjarević, Aleksandar, Sahal-Brechot, Sylvie, "Stark Widths of Spectral Lines of Neutral Neon" in Journal of Astrophysics and Astronomy, 36, no. 4 (2015):643-659,
https://doi.org/10.1007/s12036-015-9343-z .,
https://hdl.handle.net/21.15107/rcub_gery_726 .