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Stark Broadening of Ne II and Ne III Spectral Lines
Authors:M S Dimitrijević
Institution:(1) Astronomical Observatory, 7 Volgina Str., Belgrade, Serbia, 11160, Yugoslavia
Abstract:Using a semiclassical approach, the widths and shifts of the spectral lines of three Ne II and six Ne III multiplets caused by collisions with electrons, protons, and helium ions at a density of perturbing particles of 1017 cm–3 and different temperatures have been calculated. The results obtained have been compared with the known experimental and theoretical data.
Keywords:Stark broadening of spectral lines  semiclassical approach  impact width of spectral line  shift of spectral line
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