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

Abstract

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.

8 pages, 6 figures, 1 table, in press in Advances in Space Research

References in corpus (3)

• Atomic data and electron-impact broadening effect in DO white dwarf atmospheres: Si VI
• The Abundance of Boron in Diffuse Interstellar Clouds
• Stark broadening of B IV spectral lines

Cited by in corpus (1)

• Stark broadening of B IV spectral lines