SIMBAD references

2015MNRAS.454.1736D - Mon. Not. R. Astron. Soc., 454, 1736-1741 (2015/December-1)

Stark broadening of Xe VIII spectral lines.

DIMITRIJEVIC M.S., SIMIC Z., KOVACEVIC A., VALJAREVIC A. and SAHAL-BRECHOT S.

Abstract (from CDS):

Stark broadening parameters have been calculated for 60 spectral lines of Xeviii, for broadening by electron, proton, and HeIIi impacts. For calculations, the semiclassical perturbation approach in the impact approximation has been used. The widths and shifts are provided for temperatures from 20 000 K to 500 000 K and for an electron density of 10^17/ cm3. Obtained results have been used to study the influence of Stark broadening on spectral lines in DO white dwarf atmospheres and it has been found that exist broad layers where this broadening mechanism is dominant in comparison with thermal Doppler broadening.

Abstract Copyright: © 2015 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society (2015)

Journal keyword(s): atomic data - atomic processes - line: formation

VizieR on-line data: <Available at CDS (J/MNRAS/454/1736): table1.dat>

Simbad objects: 2

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