Stark broadening of B IV lines for astrophysical and laboratory plasma research

Andjelka Kova\v{c}evi\'c; Magdalena Christova; Milan S. Dimitrijevi\'c; Sylvie Sahal-Br\'echot; Zoran Simi\'c

arxiv: 1311.1330 · v1 · pith:BOE3QDTHnew · submitted 2013-11-06 · 🌌 astro-ph.SR · physics.atom-ph

Stark broadening of B IV lines for astrophysical and laboratory plasma research

Milan S. Dimitrijevi\'c , Magdalena Christova , Zoran Simi\'c , Andjelka Kova\v{c}evi\'c , Sylvie Sahal-Br\'echot This is my paper

classification 🌌 astro-ph.SR physics.atom-ph

keywords beenbroadeningstarkastrophysicalcalculateddependenceformalisminvestigate

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Stark broadening parameters for 36 multiplets of B IV have been calculated using the semi-classical perturbation formalism. Obtained results have been used to investigate the regularities within spectral series and temperature dependence.

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Stark broadening of B IV lines for astrophysical and laboratory plasma research

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