Stark broadening of Xe II lines
Astronomical Observatory, Volgina 7, 11000 Belgrade, Yugoslavia
Send offprint request to: L.Č. Popović
Accepted: 13 September 1995
We present here Stark widths and shifts for 20 Xe II multiplets which are of interest for laboratory plasma research as well as for the analysis of Hg – Mn stars spectra. For calculations the modified semiempirical approach was used. The obtained results are compared with the available experimental data.
Key words: atomic data / plasmas / stars: chemically peculiar
© European Southern Observatory (ESO), 1996