Stark broadening of spectral lines along the isoelectronic sequence of Li

1992 ◽  
Vol 45 (12) ◽  
pp. 8795-8802 ◽  
Author(s):  
S. Glenzer ◽  
N. I. Uzelac ◽  
H.-J. Kunze
Atoms ◽  
2019 ◽  
Vol 7 (1) ◽  
pp. 10
Author(s):  
Milan Dimitrijević

Rare Earth Elements are important for stellar atmosphere analysis but the corresponding Stark broadening data are scarce. For Yb III and Lu IV theoretical as well as experimental data on Stark broadening parameters of spectral lines are absent in the literature. Using the modified semiempirical method of Dimitrijević and Konjević, we determined Stark widths for four Yb III and four Lu IV transitions, belonging to the erbium isoelectronic sequence. The obtained results are also used to discuss similarities between homologous transitions in the erbium isoelectronic sequence. We note as well that calculated widths will be implemented in the STARK-B database which is also a part of the Virtual Atomic and Molecular Data Center.


Atoms ◽  
2021 ◽  
Vol 9 (2) ◽  
pp. 29
Author(s):  
Sylvie Sahal-Bréchot

The present paper revisits the determination of the semi-classical limit of the Feshbach resonances which play a role in electron impact broadening (the so-called “Stark“ broadening) of isolated spectral lines of ionized atoms. The Gailitis approximation will be used. A few examples of results will be provided, showing the importance of the role of the Feshbach resonances.


2016 ◽  
Vol 460 (2) ◽  
pp. 1658-1663 ◽  
Author(s):  
Milan S. Dimitrijević ◽  
Magdalena Christova ◽  
Zoran Simić ◽  
Andjelka Kovačević ◽  
Sylvie Sahal-Bréchot

1999 ◽  
Vol 59 (5) ◽  
pp. 374-378 ◽  
Author(s):  
B Blagojević ◽  
M V Popović ◽  
N Konjević

2021 ◽  
Vol 75 (8) ◽  
Author(s):  
Abeer Almodlej ◽  
Nabil Ben Nessib ◽  
Milan S. Dimitrijević

2000 ◽  
pp. 57-90 ◽  
Author(s):  
M.S. Dimitrijevic ◽  
S. Sahal-Brechot

Electron-, proton-, and ionized helium-impact broadening parameter tables for In II spectral lines, are presented as a function of the temperature and the perturber density. Calculations have been performed within the semiclassical perturbation approach.


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