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Stark Widths of Ar II Spectral Lines in the Atmospheres of Subdwarf B Stars

  • Published:2017-09-07 Issue:4 Volume:5 Page:26
  • ISSN:2218-2004
  • Container-title:Atoms
  • language:en
  • Short-container-title:Atoms

Author:

Hamdi Rafik,Ben Nessib Nabil,Sahal Bréchot Sylvie,Dimitrijević Milan

Publisher

MDPI AG

Subject

Condensed Matter Physics,Nuclear and High Energy Physics,Atomic and Molecular Physics, and Optics

Cited by 17 articles. 订阅此论文施引文献 订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Atomic structure, electron-impact excitation and collisional-radiative modelling for Ar II;Journal of Quantitative Spectroscopy and Radiative Transfer;2024-10

2. Stark broadening of Pd II spectral lines;Physica Scripta;2024-05-30

3. Stark broadening data for ultraviolet lines of Ni v;Monthly Notices of the Royal Astronomical Society;2024-02-07

4. Calculated Stark widths of the triply charged argon ion Ar iv;Monthly Notices of the Royal Astronomical Society;2023-10-03

5. New Ga IV, Ga V, Ge IV, and Ge V line widths for white dwarf spectra analysis: quantum mechanical results;Monthly Notices of the Royal Astronomical Society;2023-04-03
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