23 citations · 117 across the 8 of their papers we have counts for
8 papers
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 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…
Quantum Stark broadening of Ar XV lines. Strong collision and quadrupolar potential contributions
Haykel Elabidi, Sylvie Sahal-Bréchot, Milan S Dimitrijević
We present in this paper electron impact broadening for six Ar XV lines using our quantum mechanical formalism and the semiclassical perturbation one. Additionally, our calculation…
Atomic data and electron-impact broadening effect in DO white dwarf atmospheres: Si VI
R. Hamdi, N. Ben Nessib, N. Milovanović +3
Energy levels, electric dipole transition probabilities and oscillator strengths in five times ionized silicon have been calculated in intermediate coupling. The present calculatio…