Data on Stark Broadening of N VI Spectral Lines

被引：0

作者：

Dimitrijevic, Milan S. ^{[1
,2
]}

Christova, Magdalena D. ^{[3
]}

Sahal-Brechot, Sylvie ^{[2
]}

机构：

[1] Astron Observ, Volgina 7, Belgrade 11060, Serbia

[2] Sorbonne Univ, Univ PSL Paris Sci & Lettres, CNRS, LERMA Lab Etud Rayonnement & Mat Astrophys & Atmos, F-92190 Meudon, France

[3] Tech Univ Sofia, Dept Appl Phys, Sofia 1000, Bulgaria

来源：

DATA | 2024年 / 9卷 / 06期

关键词：

atomic data; Stark broadening; N VI; proton-boron fusion; line profiles; atomic processes; stellar atmospheres; WIDTHS; ELECTRONS; IONS;

D O I：

10.3390/data9060077

中图分类号：

TP [自动化技术、计算机技术];

学科分类号：

0812 ;

摘要：

Data on Stark broadening parameters, spectral line widths, and shifts for 15 multiplets of N VI, whose spectral lines are broadened by collisions with electrons, protons, alpha particles (He III) and B III, B IV, B V and B VI ions, are presented. They have been calculated using the semiclassical perturbation theory, for temperatures from 50,000 K to 2,000,000 K, and perturber densities from 10(16) cm(-3) up to 10(24) cm(-3). The data for e, p and He III are of particular interest for the analysis and modelling of atmospheres of hot and dense stars, as, e.g., white dwarfs, and for investigation of their spectra, and data for boron ions are used for analysis and modelling of laser-driven plasma in proton-boron fusion research.

引用

页数：6

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