Astron. Astrophys. Suppl. Ser.
Volume 140, Number 2, December I 1999
|Page(s)||193 - 196|
|Published online||15 December 1999|
Stark broadening of neutral zinc spectral lines*
Astronomical Observatory, Volgina 7, 11000 Belgrade, Serbia, 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: 6 September 1999
Using the semiclassical perturbation approach, we have calculated electron-, pro ton- and He II-impact line widths and shifts for 32 Zn I multiplets as a function of temperature and perturber density. Obtained results have been compared with the existing theoretical and experimental data.
Key words: atomic data / line: profiles
Table 1 is only available in electronic form: The material published electronically can be accessed: by ftp at cdsarc.u-strasbg.fr (22.214.171.124) or via http://cdsweb.u-strasbg.fr/Abstract.html
© European Southern Observatory (ESO), 1999