A&A Supplement series, Vol. 127, January II 1998, 295-297
Received November 28, 1996; accepted April 14, 1997
transitions
L.C. Popovic and M.S. Dimitrijevic
Send offprint request: L.Č. Popovic
Astronomical Observatory, Volgina 7, 11050 Beograd, Serbia,
Yugoslavia
With the development of space-borne spectroscopy, spectral line parameters
for a large number of
lines become of increasing interest for astrophysics.
To provide Stark broadening data for ion lines
from complex spectra, we present here calculated Stark widths
for 37 Kr II
lines from the 
transition. The calculations were performed by using
a modified semiempirical
approach. The obtained Stark widths are on average in
satisfactory agreement with available experimental data.
keywords: atomic data -- lines, profiles