English

Stark broadening of B IV spectral lines

Solar and Stellar Astrophysics 2016-05-25 v1

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.

Keywords

Cite

@article{arxiv.1604.08537,
  title  = {Stark broadening of B IV spectral lines},
  author = {Milan S. Dimitrijevic and Magdalena Christova and Zoran Simic and Andjelka Kovacevic and Sylvie Sahal-Brechot},
  journal= {arXiv preprint arXiv:1604.08537},
  year   = {2016}
}

Comments

6 pages, 2 figures