Stark broadening of B IV spectral lines
Milan S. Dimitrijevic, Magdalena Christova, Zoran Simic, Andjelka, Kovacevic, Sylvie Sahal-Brechot
TL;DR
This paper calculates Stark broadening parameters for B IV spectral lines using impact semiclassical perturbation formalism, analyzing their regularities and impact on white dwarf spectra.
Contribution
It introduces new Stark broadening data for B IV lines and explores their spectral regularities and effects on white dwarf observations.
Findings
Calculated Stark broadening parameters for 157 B IV multiplets.
Identified regularities within spectral series.
Demonstrated impact on B IV lines in white dwarf spectra.
Abstract
Stark broadening parameters for 157 multiplets of helium like boron (B IV) have been calculated using the impact semiclassical perturbation formalism. Obtained results have been used to investigate the regularities within spectral series. An example of the influence of Stark broadening on B IV lines in DO white dwarfs is given.
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