International audienceIn order to complete Stark broadening data for Ne II and O III lines, needed for analysis of stellar atmospheres, we determined the missing parameters for the broadening by collisions with protons and ionized helium for 15 Ne II and 5 O III multiplets. Also, electron, proton and ionized helium impact broadening parameters for an important Ne II multiplet in the visible part of the spectrum and for three Ne III multiplets were calculated. The obtained data will be included in the STARK-B database, which is a part of the Virtual Atomic and Molecular Data Center
International audienceIn the deeper layers of hot stellar photospheres the Stark widths of spectral ...
International audienceStark broadening theories and calculations have been extensively developed for...
International audienceUsing a semiclassical approach, the authors have calculated electron-, proton-...
International audienceIn order to complete Stark broadening data for Ne II and O III lines, needed f...
In order to complete Stark broadening data for Ne II, and O III lines, needed for analysis of stella...
In order to complete Stark broadening data for Ne I spectral lines which are needed for analysis of ...
Using a semiclassical approach, we have calculated electron-, proton-, He II-, Mg II-, Si II- and Fe...
International audienceUsing a semi-classical approach, we have calculated electron-, proton-, and io...
International audienceIn order to complete data on Stark broadening parameters for Ar I line in the ...
International audienceResults are presented on calculations of the electron-, proton-, and ionized h...
In order to complete data on Stark broadening parameters for Ar I line in the visible spectrum, we d...
International audienceUsing a semiclassical approach, the authors have calculated electron-, proton-...
International audienceIn the deeper layers of hot stellar photospheres the Stark widths of spectral ...
International audienceStark broadening theories and calculations have been extensively developed for...
International audienceUsing a semiclassical approach, the authors have calculated electron-, proton-...
International audienceIn order to complete Stark broadening data for Ne II and O III lines, needed f...
In order to complete Stark broadening data for Ne II, and O III lines, needed for analysis of stella...
In order to complete Stark broadening data for Ne I spectral lines which are needed for analysis of ...
Using a semiclassical approach, we have calculated electron-, proton-, He II-, Mg II-, Si II- and Fe...
International audienceUsing a semi-classical approach, we have calculated electron-, proton-, and io...
International audienceIn order to complete data on Stark broadening parameters for Ar I line in the ...
International audienceResults are presented on calculations of the electron-, proton-, and ionized h...
In order to complete data on Stark broadening parameters for Ar I line in the visible spectrum, we d...
International audienceUsing a semiclassical approach, the authors have calculated electron-, proton-...
International audienceIn the deeper layers of hot stellar photospheres the Stark widths of spectral ...
International audienceStark broadening theories and calculations have been extensively developed for...
International audienceUsing a semiclassical approach, the authors have calculated electron-, proton-...