Using the semi-classical perturbation approach in the impact approximation, full width at half maximum and shift have been determined for eight spectral lines of Ar VII, for broadening by electron-, proton-, and He III-impacts. The results are provided for temperatures from 20,000 K to 500,000 K, and for an electron density of 10(18) cm(-3). The obtained results will be included in the STARK-B database, which is also in the virtual atomic and molecular data center (VAMDC)
In order to complete Stark broadening data for Ne II, and O III lines, needed for analysis of stella...
Stark broadening theory is currently operated for calculating widths and shifts of spectral lines th...
Stark broadening theory is currently operated for calculating widths and shifts of spectral lines th...
Using the semi-classical perturbation approach in the impact approximation, full width at half maxim...
Using the semi-classical perturbation approach in the impact approximation, full width at half maxim...
Using the semi-classical perturbation approach in the impact approximation, full width at half maxim...
Stark broadening parameters, full width at half maximum of spectral line and shift, have been calcul...
Stark broadening parameters have been calculated for 60 spectral lines of Xe VIII, for broadening by...
Stark broadening parameters have been calculated for 60 spectral lines of Xe VIII, for broadening by...
We present in this paper the results of a theoretical study of electron impact broadening for severa...
International audienceIn order to complete data on Stark broadening parameters for Ar I line in the ...
International audienceIn order to complete data on Stark broadening parameters for Ar I line in the ...
International audienceIn order to complete data on Stark broadening parameters for Ar I line in the ...
International audienceIn order to complete data on Stark broadening parameters for Ar I line in the ...
In order to complete data on Stark broadening parameters for Ar I line in the visible spectrum, we d...
In order to complete Stark broadening data for Ne II, and O III lines, needed for analysis of stella...
Stark broadening theory is currently operated for calculating widths and shifts of spectral lines th...
Stark broadening theory is currently operated for calculating widths and shifts of spectral lines th...
Using the semi-classical perturbation approach in the impact approximation, full width at half maxim...
Using the semi-classical perturbation approach in the impact approximation, full width at half maxim...
Using the semi-classical perturbation approach in the impact approximation, full width at half maxim...
Stark broadening parameters, full width at half maximum of spectral line and shift, have been calcul...
Stark broadening parameters have been calculated for 60 spectral lines of Xe VIII, for broadening by...
Stark broadening parameters have been calculated for 60 spectral lines of Xe VIII, for broadening by...
We present in this paper the results of a theoretical study of electron impact broadening for severa...
International audienceIn order to complete data on Stark broadening parameters for Ar I line in the ...
International audienceIn order to complete data on Stark broadening parameters for Ar I line in the ...
International audienceIn order to complete data on Stark broadening parameters for Ar I line in the ...
International audienceIn order to complete data on Stark broadening parameters for Ar I line in the ...
In order to complete data on Stark broadening parameters for Ar I line in the visible spectrum, we d...
In order to complete Stark broadening data for Ne II, and O III lines, needed for analysis of stella...
Stark broadening theory is currently operated for calculating widths and shifts of spectral lines th...
Stark broadening theory is currently operated for calculating widths and shifts of spectral lines th...