Issue |
Astron. Astrophys. Suppl. Ser.
Volume 129, Number 1, April I 1998
|
|
---|---|---|
Page(s) | 155 - 156 | |
DOI | https://doi.org/10.1051/aas:1998395 | |
Published online | 15 April 1998 |
Stark broadening of spectral lines of multicharged ions of astrophysical interest*
XVIII. Si XI and Si XIII 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 CNRS 812, Observatoire de Paris-Meudon, 92190 Meudon, France
Send offprint request to: M.S. Dimitrijević
Received:
18
August
1997
Accepted:
3
September
1997
Using a semiclassical perturbation
approach, we have
calculated electron-, pro ton-, and
He III- im pact line widths and shifts for 4 Si XI multiplets
for perturber densities 1018- 1023 cm-3 and temperatures
K,
and for 61 Si XIII multiplets
for perturber densities 1016- 1023 cm-3 and temperatures
K.
For lower perturber
densities, obtained results are linear with perturber density.
Key words: lines: profile / atomic data / plasmas
© European Southern Observatory (ESO), 1998