Astronomy and Astrophysics – Astronomy
Scientific paper
Jun 1981
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981mnras.195..705d&link_type=abstract
Monthly Notices of the Royal Astronomical Society, vol. 195, June 1981, p. 705-719. NATO-supported research.
Astronomy and Astrophysics
Astronomy
87
Iron, Line Spectra, Plasma Spectra, Rarefied Plasmas, Atomic Spectra, Electron Energy, Plasma Resonance, Plasma Temperature
Scientific paper
Wavelengths and intensities of dielectronic satellite lines of the type 1snl-2pnl have been calculated for n equals 2, 3 and 4 in iron. These are compared with previous calculations for n equals 2. The effect of cascades from higher satellite levels is shown to be negligible. An approximation is used to scale for all n greater than 4, in order to produce the total satellite spectrum, including the contribution to the apparent resonance line intensity. A technique is proposed for using this spectrum to measure the electron temperature in the source. An estimate is made of the dielectronic recombination rate, which is compared with the result of earlier semi-empirical formulae.
Dubau Jacques
Gabriel Alan H.
Loulergue M.
Steenman-Clark Lois
Volonte Sergio
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