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A&A Supplement series, Vol. 127, February I 1998, 543-544

Received May 23; accepted May 27, 1997

Stark broadening of spectral lines of multicharged ions of astrophysical interest

XVI. S V spectral linesgif

M.S. Dimitrijevictex2html_wrap665 and S. Sahal-Bréchottex2html_wrap667

tex2html_wrap669  Astronomical Observatory, Volgina 7, 11050 Belgrade, Yugoslavia
tex2html_wrap671  Laboratoire "Astrophysique, Atomes et Molécules", Département Atomes et Molécules en Astrophysique, Unité associée au CNRS No. 812, Observatoire de Paris-Meudon, 92190 Meudon, France


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 tex2html_wrap_inline657 and temperatures tex2html_wrap_inline659. For lower perturber densities, the obtained results are linear with perturber density.

keywords: lines: profile -- atomic data

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