Issue |
Astron. Astrophys. Suppl. Ser.
Volume 127, Number 3, February I 1998
|
|
---|---|---|
Page(s) | 543 - 544 | |
DOI | https://doi.org/10.1051/aas:1998375 | |
Published online | 15 February 1998 |
Stark broadening of spectral lines of multicharged ions of astrophysical interest*
XVI. S V 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 No. 812, Observatoire de Paris-Meudon, 92190 Meudon, France
Received:
23
May
1997
Accepted:
27
May
1997
Using a semiclassical
approach, we have
calculated electron-, proton-, and
He III-impact line widths and shifts for 34 S V multiplets
for perturber densities
and temperatures
. For lower perturber
densities, the obtained results are linear with perturber density.
Key words: lines: profile / atomic data
© European Southern Observatory (ESO), 1998