Using the semiclassical perturbation method, electron-, proton-, and ionized helium-impact line widths and shifts for the nine Cr
International audienceUsing semiclassical perturbation approach in the impact approximation, we have...
International audienceIn order to provide Stark broadening data in X-ray and far UV wavelength regio...
By using the semiclassical-perturbation formalism, we have calculated e lec tron-, proton-, and He I...
Electron-, proton-, and ionized helium-impact broadening parameter tables for In II spectral lines, ...
International audienceUsing a semiclassical approach, the authors have calculated electron-, proton-...
International audienceIn order to complete data on Stark broadening parameters for Ar I line in the ...
Using the semiclassical perturbation formalism, we have calculated electron-, proton-, and ionize...
Using the semi-classical perturbation approach in the impact approximation, full width at half maxim...
In order to complete data on Stark broadening parameters for Ar I line in the visible spectrum, we d...
Stark broadening parameters, full width at half maximum of spectral line and shift, have been calcul...
Using a semiclassical approach, we have calculated electron-, proton-, and ionized helium-impact l...
International audienceUsing a semiclassical approach, the authors have calculated electron-, proton-...
International audienceStark broadening parameters, full widths at half intensity maximum and shifts ...
International audienceNew Stark broadening parameters of interest for the astrophysical, laboratory ...
International audienceUsing semiclassical perturbation approach in the impact approximation, we have...
International audienceIn order to provide Stark broadening data in X-ray and far UV wavelength regio...
By using the semiclassical-perturbation formalism, we have calculated e lec tron-, proton-, and He I...
Electron-, proton-, and ionized helium-impact broadening parameter tables for In II spectral lines, ...
International audienceUsing a semiclassical approach, the authors have calculated electron-, proton-...
International audienceIn order to complete data on Stark broadening parameters for Ar I line in the ...
Using the semiclassical perturbation formalism, we have calculated electron-, proton-, and ionize...
Using the semi-classical perturbation approach in the impact approximation, full width at half maxim...
In order to complete data on Stark broadening parameters for Ar I line in the visible spectrum, we d...
Stark broadening parameters, full width at half maximum of spectral line and shift, have been calcul...
Using a semiclassical approach, we have calculated electron-, proton-, and ionized helium-impact l...
International audienceUsing a semiclassical approach, the authors have calculated electron-, proton-...
International audienceStark broadening parameters, full widths at half intensity maximum and shifts ...
International audienceNew Stark broadening parameters of interest for the astrophysical, laboratory ...
International audienceUsing semiclassical perturbation approach in the impact approximation, we have...
International audienceIn order to provide Stark broadening data in X-ray and far UV wavelength regio...
By using the semiclassical-perturbation formalism, we have calculated e lec tron-, proton-, and He I...
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