Free Access
Issue
Astron. Astrophys. Suppl. Ser.
Volume 119, Number 2, October_II 1996
Page(s) 369 - 371
DOI https://doi.org/10.1051/aas:1996250
Published online 15 October 1996
Stark broadening of spectral lines of multicharged ions of astrophysical interest. XIV. Be III and B III DOI: 10.1051/aas:1996250

Astronomy and Astrophysics Supplement Series, Vol. 119, October II 1996, 369-371

Stark broadening of spectral lines of multicharged ions of astrophysical interest. XIV. Be III and B III

M.S. Dimitrijevic and S. Sahal-Bréchot Send offprint requests to: M.S. Dimitrijevic

Astronomical Observatory, Volgina 7, 11050 Beograd, Yugoslavia
Laboratoire ``Astrophysique, Atomes et Molécules" Département Atomes et Molécules en Astrophysique Unité associée au C.N.R.S. No. 812, Observatoire de Paris-Meudon, 92190 Meudon, France

Received February 20; accepted March 15, 1996

Abstract:

Using a semiclassical approach, we have calculated electron-, proton-, and ionized helium-impact line widths and shifts for 12 Be III and 27 B III multiplets. The obtained results have been compared with available experimental and theoretical data.

Key words: lines: profiles-atomic and molecular data


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