Stark broadening of B IV spectral lines
arXiv:1604.08537 · doi:10.1093/mnras/stw1023
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.
6 pages, 2 figures
References in corpus (4)
- High-resolution FUSE and HST ultraviolet spectroscopy of the white dwarf central star of Sh 2-216
- Atomic data and electron-impact broadening effect in DO white dwarf atmospheres: Si VI
- Stark broadening data for spectral lines of rare-earth elements: Nb III
- Stark broadening of B IV lines for astrophysical and laboratory plasma research