Nonequilibrium Non-Lte Ionization in Supernova Remnants

Details Nonequilibrium Non-Lte Ionization in Supernova Remnants Nonequilibrium Non-Lte Ionization in Supernova Remnants

Feb 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992a%26a...254..460b&link_type=abstract

Astronomy and Astrophysics, Vol.254, NO. FEB(I), P. 460, 1992

Astronomy and Astrophysics

Astrophysics

3

Supernova Remnants, X-Rays: Spectroscopy, Atomic And Molecular Processes

Scientific paper

The coincidence of all relevant time scales in young supernova remnants, from the macroscopic life time of the SNR to the microscopic ionization- and energy transfer time scales can cause non-LTE configurations of the local electron distribution function. For a pure iron plasma with electron temperatures in the range Te = l07 - l08 K we determine the shape of the equilibrium electron distribution function including ionization- and recombination effects and discuss its influence on the energy transfer rate and ionization structure of the gas.

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