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Astron. Astrophys. Suppl. Ser. 130, 539-540

Stark broadening of spectral lines of multicharged ions of astrophysical interest

XIX. Na X spectral lines[*]

M.S. Dimitrijevic1 and S. Sahal-Bréchot2

Send offprint request: M.S. Dimitrijevi

1- Astronomical Observatory, Volgina 7, 11050 Belgrade, Yugoslavia
2- Laboratoire "Astrophysique, Atomes et Molécules", Département Atomes et Molécules en Astrophysique, Unité associée au CNRS 812, Observatoire de Paris-Meudon, 92190 Meudon, France

Received December 17; accepted December 18, 1997


Using a semiclassical perturbation approach, we have calculated electron-, proton-, and He III-impact line widths and shifts for 57 Na X multiplets for perturber densities 1017- 1024 cm-3 and temperatures T = 200 000 - 5 000 000 K. For lower perturber densities, the Stark broadening parameters are proportional to the perturber density.

Key words: lines: profile-atomic data

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