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Addendum: STARK BROADENING PARAMETER TABLES FOR Be I LINES OF ASTROPHYSICAL INTEREST。
STARK BROADENING PARAMETER TABLES FOR Ne VIII AND Na IX LINES OF ASTROPHYSICAL INTEREST。
STARK BROADENING PARAMETER TABLES FOR Al XI AND Si XII LINES OF ASTROPHYSICAL INTEREST。
Errata: STARK BROADENING PARAMETER TABLES FOR Mg I LINES OF INTEREST FOR SOLAR AND STELLAR SPECTRA RESEARCH I
STARK BROADENING PARAMETER TABLES FOR O IV AND O V LINES OF ASTROPHYSICAL IMPORTANCE。
Using a semiclassical approach, we have calculated electron-, proton-, and ionized helium-impact line widths and shifts for 20 In III multiplets for perturber densities 1014− 1020 cm−3 a...
Using a semiclassical approach, we have calculated electron−, proton−, and He IIIimpact line widths and shifts for 6 Kr VIII multiplets as a function of temperature and perturber ...
Using the semiclassical perturbation formalism, we have calculated electron-, proton-, and ionized helium-impact line widths and shifts for six Au I lines as a function of temperature and perturber ...
Using a semiclassical approach, we have calculated electron−, proton−, He II−, Mg II-, Si II- and Fe II-impact line widths and shifts for 189 Ca I multiplets as a function of tempe...
Using a semiclassical approach, we have calculated electron−, protonand He IIimpact line widths and shifts for 32 Zn I multiplets as a function of temperature and perturber dens...
Using a semiclassical approach, we have calculated electron−, proton−, and He IIIimpact line widths and shifts for 9 Ar VIII transitions as a function of temperature and perturber...
In order to provide the Stark broadening data for ion lines from complex spectra, here we present calculated Stark widths and shifts for 37 Kr II lines. The calculations were performed by using the ...
Electron-, proton-, and ionized helium-impact broadening parameter tables for neutral calcium spectral lines, have been presented as a function of the temperature and the perturber density. Calculat...

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