Issue |
Astron. Astrophys. Suppl. Ser.
Volume 140, Number 2, December I 1999
|
|
---|---|---|
Page(s) | 193 - 196 | |
DOI | https://doi.org/10.1051/aas:1999417 | |
Published online | 15 December 1999 |
Stark broadening of neutral zinc spectral lines*
1
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
Received:
24
June
1999
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
© European Southern Observatory (ESO), 1999