Aims. The aim of this work is to provide Stark parameters of low intensity Xe II and Xe III spectral lines from which scarce or null previous information exist.This work completes the measurements of ionized Xenon parameters developed in the last few years and extends Stark parameters database for astrophysical applications. Methods. All Stark parameters were measured in a pulsed arc plasma with 95% of helium and 5% of xenon. Measured electron densities and temperatures were in the range of (0.2-1.7)$\times$1023 m-3 and 18 000-25 500 K, respectively. Results. As a whole 25 Stark widths and 29 shifts of Xe II spectral lines have been measured, along with 10 Stark widths and 6 shifts of Xe III. Some of the presented data are c...
Context. The Stark broadening of the spectral lines of the wavelengths 501.6, 667.8, 728.1, 388.9, 5...
Context. The Stark broadening of the spectral lines of the wavelengths 501.6, 667.8, 728.1, 388.9, 5...
Stark widths and shifts of astrophysically important 10 doubly ionized sulfur (S III) spectral line...
Stark broadening parameters (widths and shifts) of two He I isolated spectral lines are measured in...
Aims.Our aims is to measure with good accuracy the Stark parameters (width and shift) of the He I 31...
Stark widths $(W)$ and shifts $(d)$ of 5 singly ionized fluorine (F II) spectral lines within the $\...
Stark width (W) and shift (d) of the neutral helium (He I) 381.96 nm spectral line in the high lyi...
Context. Stark broadening of the 447.1 line of neutral helium in a weakly coupled plasma has been st...
Context. The Stark broadening of the spectral lines of the wavelengths 501.6, 667.8, 728.1, 388.9, 5...
The Stark widths and shifts of 18 triply ionized argon (Ar IV) spectral lines have been measured at ...
Context. Stark broadening of the 447.1 line of neutral helium in a weakly coupled plasma has been st...
The Stark widths and shifts of 18 triply ionized argon (Ar IV) spectral lines have been measured at ...
8 pags., 5 figs., 3 tabs. -- 25th Summer School and International Symposium on the Physics of Ionize...
The Stark widths and shifts of 18 triply ionized argon (Ar IV) spectral lines have been measured at ...
We present here Stark widths and shifts for 20 Xe II multiplets which are of interest for laborator...
Context. The Stark broadening of the spectral lines of the wavelengths 501.6, 667.8, 728.1, 388.9, 5...
Context. The Stark broadening of the spectral lines of the wavelengths 501.6, 667.8, 728.1, 388.9, 5...
Stark widths and shifts of astrophysically important 10 doubly ionized sulfur (S III) spectral line...
Stark broadening parameters (widths and shifts) of two He I isolated spectral lines are measured in...
Aims.Our aims is to measure with good accuracy the Stark parameters (width and shift) of the He I 31...
Stark widths $(W)$ and shifts $(d)$ of 5 singly ionized fluorine (F II) spectral lines within the $\...
Stark width (W) and shift (d) of the neutral helium (He I) 381.96 nm spectral line in the high lyi...
Context. Stark broadening of the 447.1 line of neutral helium in a weakly coupled plasma has been st...
Context. The Stark broadening of the spectral lines of the wavelengths 501.6, 667.8, 728.1, 388.9, 5...
The Stark widths and shifts of 18 triply ionized argon (Ar IV) spectral lines have been measured at ...
Context. Stark broadening of the 447.1 line of neutral helium in a weakly coupled plasma has been st...
The Stark widths and shifts of 18 triply ionized argon (Ar IV) spectral lines have been measured at ...
8 pags., 5 figs., 3 tabs. -- 25th Summer School and International Symposium on the Physics of Ionize...
The Stark widths and shifts of 18 triply ionized argon (Ar IV) spectral lines have been measured at ...
We present here Stark widths and shifts for 20 Xe II multiplets which are of interest for laborator...
Context. The Stark broadening of the spectral lines of the wavelengths 501.6, 667.8, 728.1, 388.9, 5...
Context. The Stark broadening of the spectral lines of the wavelengths 501.6, 667.8, 728.1, 388.9, 5...
Stark widths and shifts of astrophysically important 10 doubly ionized sulfur (S III) spectral line...