Stark broadening of spectral lines of multicharged ions of astrophysical interest^*

XVI. S V spectral lines

¹ Astronomical Observatory, Volgina 7, 11050 Belgrade, Yugoslavia
² Laboratoire "Astrophysique, Atomes et Molécules", Département Atomes et Molécules en Astrophysique, Unité associée au CNRS No. 812, Observatoire de Paris-Meudon, 92190 Meudon, France

Received: 23 May 1997
Accepted: 27 May 1997

Abstract

Using a semiclassical approach, we have calculated electron-, proton-, and He III-impact line widths and shifts for 34 S V multiplets for perturber densities and temperatures . For lower perturber densities, the obtained results are linear with perturber density.