Astron. Astrophys. Suppl. Ser.
Volume 128, Number 1, February II 1998
|Page(s)||203 - 205|
|Published online||15 February 1998|
The electron impact broadening parameters in hot star atmospheres: Mn II, Mn III, Ga III, Ge III and Ge IV lines*
Astronomical Observatory, Volgina 7, 11050 Beograd, Serbia, Yugoslavia
Send offprint request to: L.Č. Popović
Accepted: 6 June 1997
The electron - impact line widths and shifts for 16 Mn II, 3 Mn III, 10 Ga III, 8 Ge III and 14 Ge IV multiplets, have been considered within a modified semiempirical approach. Moreover, using a semiclassical approach, we have considered electron-, pro ton-, and He III-im pact line widths and shifts for 3 Ge IV multiplets. The obtained results have been compared with other theoretical results.
Key words: lines: profile-atomic data / stars: chemically peculiar
Tables 1-4 are only available in electronic form via anonymous ftp 188.8.131.52 at the CDS in Strasbourg or via http:// cdsweb.u-strasbg.fr/Abstract.html
© European Southern Observatory (ESO), 1998