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.
Keywords:
Stark broadening / atomic data / Ne I: line profiles
Source:
Journal of Astrophysics and Astronomy, 2015, 36, 4, 643-659
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 - convd_1592
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 = "convd_1592"
}
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
convd_1592
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
convd_1592 .
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 .,
convd_1592 .
