Issue |
Astron. Astrophys. Suppl. Ser.
Volume 122, Number 1, April I 1997
|
|
---|---|---|
Page(s) | 163 - 166 | |
DOI | https://doi.org/10.1051/aas:1997299 | |
Published online | 15 April 1997 |
Stark broadening of Ba I and Ba II spectral lines*
1
Astronomical Observatory, Volgina 7, 11050 Belgrade, Serbia, 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:
11
June
1996
Accepted:
14
June
1996
Using a semiclassical
approach, we have
calculated electron-, pro ton-, and
ionized he li um- im pact line widths and shifts for 14 Ba I and
64 Ba II multiplets
for perturber densities 1015- 1018 cm-3
and temperatures K for Ba I and
K for Ba II. The results have been
compared with available experimental and theoretical data.
Key words: line: profiles-atomic data
© European Southern Observatory (ESO), 1997