Issue |
Astron. Astrophys. Suppl. Ser.
Volume 119, Number 2, October II 1996
|
|
---|---|---|
Page(s) | 369 - 371 | |
DOI | https://doi.org/10.1051/aas:1996250 | |
Published online | 15 October 1996 |
Stark broadening of spectral lines of multicharged ions of astrophysical interest. XIV. Be III and B III
1
Astronomical Observatory, Volgina 7, 11050 Beograd, 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:
20
February
1996
Accepted:
15
March
1996
Using a semiclassical approach, we have calculated electron-, proton-, and ionized helium-impact line widths and shifts for 12 Be III and 27 B III multiplets. The obtained results have been compared with available experimental and theoretical data.
Key words: lines: profiles-atomic and molecular data
© European Southern Observatory (ESO), 1996