299 citations · 406 across the 9 of their papers we have counts for
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The STARK-B database as a resource for \textquotedblleft STARK" widths and shifts data: State of advancement and program of development
Sylvie Sahal-Bréchot, Milan S. Dimitrijević, Nicolas Moreau +1
\textquotedblleft Stark" broadening theories and calculations have been extensively developed for about 50 years and can now be applied to many needs, especially for accurate spect…
The OIV 1407.3Å/1401.1Å emission-line ratio in a plasma
Nabil Ben Nessib, Norah Alonizan, Rabia Qindeel +2
Line ratio of O IV 1407.3 Å/1401.1 Å\- is calculated using mostly our own atomic and collisional data. Energy levels and oscillator strengths needed for this calculation have been…
Stark broadening data for spectral lines of rare-earth elements: Nb III
Zoran Simić, Milan S. Dimitrijević, Luka Č. Popović
The electron-impact widths for 15 doubly charged Nb ion lines have been theoretically determined by using the modified semiempirical method. Using the obtained results, we consider…
Stark widths of Ar III spectral lines in the atmospheres of subdwarf B stars
Rafik Hamdi, Nabil Ben Nessib, Sylvie Sahal-Bréchot +1
Using semiclassical perturbation approach in impact approximation, we have calculated Stark widths for 32 spectral lines of doubly charged argon (Ar III). Oscillator strengths are…
Stark broadening of B IV lines for astrophysical and laboratory plasma research
Milan S. Dimitrijević, Magdalena Christova, Zoran Simić +2
Stark broadening parameters for 36 multiplets of B IV have been calculated using the semi-classical perturbation formalism. Obtained results have been used to investigate the regul…
Stark Broadening of Carbon and Oxygen Lines in Hot DQ White Dwarf Stars: Recent Results and Applications
P. Dufour, N. Ben Nessib, S. Sahal-Bréchot +1
White dwarf stars are traditionally found to have surface compositions made primarily of hydrogen or helium. However, a new family has recently been uncovered, the so-called Hot DQ…