J/A+AS/119/369 J/A+AS/119/369 Stark broadening. XIV: Be III and B III M S Dimitrijevic S Sahal-Brechot Astron. Astrophys. Suppl. Ser. 119 369 1996 1996A&AS..119..369D VI/82 : Stark broadening of H lines J/A+AS/105/243 : Stark broadening of BeI lines J/A+AS/105/245 : Stark broadening Al XI and Si XII J/A+AS/107/349 : Stark broadening of Ne VIII and Na IX J/A+AS/109/551 : Stark broadening of OIV and OV J/A+AS/115/351 : Stark broadening of C V and P V J/A+AS/116/359 : Stark broadening of Xe II lines J/A+AS/119/529 : Stark broadening of Sr I spectral lines J/A+AS/120/373 : Stark width in Sc II, Y II and Zr II spectra J/A+AS/122/163 : Stark broadening of Ba I and Ba II lines J/A+AS/122/533 : Stark broadening of P IV spectral lines Atomic physics atomic data line: profiles molecular data 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.

N Perturber density cm-3 El Element name --- Tr Transition --- lambda Wavelength 0.1nm C Parameter C number=1 C/FWHM gives an estimate of the maximum perturber density for which the line may be treated as isolated and tabulated data may be used 0.1nm/cm3 T Temperature K n_We (4) --- We FWHM for electron impacts number=2 FWHM denotes Full Width at Half Maximum 0.1nm n_de (4) --- de shift for electron impacts number=3 A positive (resp. negative) shift is towards the red (resp. blue) 0.1nm n_Wp (4) --- Wp FWHM for proton impacts (2) number=5 Values for NV > 0.5 are not given, because in this case the impact approximation is no longer valid 0.1nm n_dp (4) --- dp shift for proton impacts (3) number=5 Values for NV > 0.5 are not given, because in this case the impact approximation is no longer valid 0.1nm n_WHe+ (4) --- WHe+ FWHM for He II-impacts number=2 FWHM denotes Full Width at Half Maximum 0.1nm n_dHe+ (4) --- dHe+ shift for He II-impacts number=3 A positive (resp. negative) shift is towards the red (resp. blue) 0.1nm Patricia Bauer CDS 1996Apr02Milan S. Dimitrijevic <mdimitrijevic@aob.aob.bg.ac.yu> J_A+AS_119_369.xml