Issue |
Astron. Astrophys. Suppl. Ser.
Volume 119, Number 3, November I 1996
|
|
---|---|---|
Page(s) | 529 - 530 | |
DOI | https://doi.org/10.1051/aas:1996265 | |
Published online | 15 November 1996 |
Stark broadening of Sr I spectral lines
1
Astronomical Observatory, Volgina 7, 11050 Belgrade, Yugoslavia
2
Laboratoire “Astrophysique, Atomes et Molécules", Département Atomes et Molécules en Astrophysique, Unité associée au C.N.R.S. No. 812, Observatoire de Paris-Meudon, 92190 Meudon, France
Send offprint request to: M.S. Dimitrijević
Received:
13
March
1996
Accepted:
26
March
1996
Using a semiclassical approach, we have calculated electron-, proton-, and ionized helium-impact line widths and shifts for 33 Sr I multiplets for perturber densities 1013 cm-3 (for stellar plasma research) and 1015- 1018 cm-3 (for laboratory plasma research) and temperatures T = 2 500 - 50 000 K.
Key words: lines: profile-atomic data
© European Southern Observatory (ESO), 1996