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,
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