activity
20032012
most citedSemi-classical theory of collisional depolarization of spectral lines by atomic hydrogen. I: application to p states of neutral atoms

42 citations · 91 across the 10 of their papers we have counts for

collaborators

10 papers

physics.atom-ph2012★ 1 cited

Cross Sections for Electron Impact Excitation of O VI Lines

Haykel Elabidi, Sylvie Sahal-Bréchot, Nébil Ben Nessib

Radiative atomic data and electron impact excitation cross sections for the transitions in O VI for transitions among the fine structure levels belonging to the …

astro-ph.SR2012★ 2 cited

Stark Broadening of in III Lines in Astrophysical and Laboratory Plasma

Z. Simic, M. S. Dimitrijevic, A. B. Kovacevic +1

Besides the need of Stark broadening parameters for a number of problems in physics, and plasma technology, in hot star atmospheres the conditions exist where Stark widths are comp…

astro-ph.SR2012★ 22 cited

Comparisons and Comments on Electron and Ion Impact Profiles of Spectral Lines

Sylvie Sahal-Brechot, Milan S. Dimitrijevic, Nebil Ben Nessib

Stark broadening theory is currently operated for calculating widths and shifts of spectral lines that are needed for spectroscopic diagnostics and modelling in astrophysics, labor…

astro-ph.SR2012★ 1 cited

Stark Broadening and White Dwarfs

Milan S. Dimitrijevic, Andjelka Kovacevic, Zoran Simic +1

White dwarf and pre-white dwarf atmospheres are one of the best examples for the application of Stark broadening research results in astrophysics, due to plasma conditions very fav…

astro-ph.SR2012★ 4 cited

Stark Broadening of several Ar I Spectral Lines in the Visible Part of the Spectrum

Milan S. Dimitrijevic, Andjelka Kovacevic, Zoran Simic +1

In order to complete data on Stark broadening parameters for Ar I line in the visible spectrum, we determined Stark widths and shifts due to electron, proton, and ionized helium im…

astro-ph.SR2012★ 3 cited

Stark Broadening of several Ne II, Ne III and O III Spectral Lines for the Stark-B Database

Milan S. Dimitrijevic, Andjelka Kovacevic, Zoran Simic +1

In order to complete Stark broadening data for Ne II, and O III lines, needed for analysis of stellar atmospheres, we determined, within the semiclassical perturbation method, the…