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Zr II & III electron-impact broadening parameters
The electron-impact widths for 30 Zr III lines were calculated using the modified semi-empirical (MSE) method. For two Zr II and four Zr III astrophysically important UV lines,... -
Co III electron-impact broadening parameters
In hot star atmospheres, the Stark broadening mechanism is the main pressure broadening mechanism. An interesting application where such a mechanism is of interest is the... -
Stark broadening of Be III lines
Using a semiclassical perturbation method, we have calculated electron-, proton-, and ionized helium-impact line widths and shifts for 52 Be III multiplets as a function of... -
Cd III Stark broadening parameters
Stark broadening parameters, widths and shifts, for 84 spectral lines of doubly-ionized cadmium (Cd III) have been calculated using the modified semi-empirical approach (MSE).... -
Stark broadening of Si V
Using a semiclassical perturbation approach, we have obtained Stark broadening parameters for 16 Si V multiplets using atomic data calculated ab initio with the SUPERSTRUCTURE... -
Stark broadening of Ga I spectral lines
Stark broadening of the 18 Ga I transitions has been analyzed within the framework of the semiclassical perturbation method. Results obtained have been compared with available... -
O II Stark broadening parameters
Using a modified semiempirical approach, we have calculated Stark broadening full widths at half maximum for 25 OII multiplets for temperatures from 5000K up to 80000K using the... -
Stark broadening of Cd I spectral lines
Stark broadening parameters, widths, and shifts for 33 CdI singlets and 37 triplets were calculated using the semiclassical perturbation method. The results were compared with... -
Stark broadening X.
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Stark broadening. XII. OIV & OV
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Stark broadening. XIII. C V and P V
Using a semiclassical approach, we have calculated electron-, proton-, and He III-impact line widths and shifts for 25 C V and 51 P V multiplets. -
Xe II lines Stark broadening
We present here Stark widths and shifts for 20 Xe II multiplets which are of interest for laboratory plasma research as well as for the analysis of Hg-Mn stars spectra. For... -
Stark broadening. XIV: Be III and B III
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... -
Stark broadening : Sr I
Using a semiclassical approach, we have calculated electron-, proton-, and ionized helium-impact line widths and shifts for 33 Sr I multiplets for perturber densities... -
Sc II, Y II & Zr II Stark width
Here we present Stark widths for some astrophysically important ns-np transitions of Sc II, Y II and Zr II. Stark widths were calculated within the modified semiempirical... -
Ba I & Ba II Stark broadening
Using a semiclassical approach, we have calculated electron-, proton-, and ionized helium-impact line widths and shifts for 14 Ba I and 64 Ba II multiplets for perturber... -
Stark broadening of P IV spectral lines
Using a semiclassical approach, we have calculated electron-, proton-, and He III-impact line widths and shifts for 114 P IV multiplets for perturber densities... -
Stark broadening of Kr II lines
With the development of space-borne spectroscopy, spectral line parameters for a large number of lines become of increasing interest for astrophysics. To provide Stark... -
Stark broadening of S V lines
Using a semiclassical approach, we have calculated electron-, proton-, and He III-impact line widths and shifts for 34 S V multiplets for perturber densities 10^17^-10^21^cm^-3^... -
Stark broadening of Mn, Ga & Ge multiplets
The electron - impact line widths and shifts for 16 Mn II, 3 Mn III, 10 Ga III, 8 Ge III and 14 Ge IV multiplets, have been considered within a modified semiempirical approach....
