Astron. Astrophys. Suppl. Ser.
Volume 133, Number 2, December I 1998
|Page(s)||227 - 228|
|Published online||15 December 1998|
Stark broadening of spectral lines of multicharged ions of astrophysical interest*
XXII. K VIII and K IX spectral lines
Astronomical Observatory, Volgina 7, 11050 Belgrade, Yugoslavia
2 Laboratoire "Astrophysique, Atomes et Molécules", Département Atomes et Molécules en Astrophysique, Unité associée au CNRS 812, Observatoire de Paris-Meudon, 92190 Meudon, France
Send offprint request to: M.S. Dimitrijević
Accepted: 4 June 1998
By using the semiclassical-perturbation formalism, we have calculated e lec tron-, proton-, and He III-impact line widths and shifts for 4 K VIII and 30 K IX multiplets, of interest for analysis, investigation and modeling of different plasmas in solar and stellar subphotospheric layers research and plasma physics. The obtained results are presented as a function of temperature and perturber density. Results are compared with other theoretical estimates, based on regularities and systematic trends.
Key words: lines: profile-atomic data
Tables 1–2 are only available in electronic form at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (22.214.171.124) or via http://cdsweb.u-strasbg.fr/Abstract.html
© European Southern Observatory (ESO), 1998