Astronomy and Astrophysics – Astrophysics
Scientific paper
Sep 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990apj...360..737l&link_type=abstract
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 360, Sept. 10, 1990, p. 737-740.
Astronomy and Astrophysics
Astrophysics
12
Atomic Spectra, Cosmic Plasma, Iron, Line Spectra, Stark Effect, Temperature Dependence, Chemical Composition, Electron Density (Concentration)
Scientific paper
Stark broadening parameters of iron lines from the a 5G0 - e 5H multiplet (1146) and the z 3G0 - e 3H multiplet (1165) transition arrays are presented for temperatures ranging from 6500 to 14,100 K. Stark width is plotted against temperature for the Fe I 5383.371 A line. Temperatures, pressures, electron densities, and line profiles are determined and compared with experimental data.
Lebrun Jean-Luc
Lesage Alain
Richou Jacques
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