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DOI: 10.1051/aas:1998136
A&A Supplement series, Vol. 128, February II 1998, 203-205
Received June 5; accepted June 6, 1997
The electron impact broadening parameters in
hot star
atmospheres: Mn II, Mn III, Ga III, Ge III and Ge IV lines
L.C. Popovic and M.S. Dimitrijevic
Send offprint request: L.C. Popovic
Astronomical Observatory, Volgina 7, 11050 Beograd, Serbia,
Yugoslavia
Abstract:
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-, proton-, and He III-impact line widths and shifts for 3 Ge IV multiplets. The obtained results have been compared with other theoretical results.
keywords: lines: profile-atomic data -- stars: chemically peculiar
Tables at the CDSCopyright by the European Southern Observatory (ESO)
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