Non-relativistic Free-Free Emission due to the n-distribution of Electrons-Radiative Cooling and Thermally Averaged and Total Gaunt Factors

Tracking the thermal evolution of plasmas, characterized by an n-distribution, using numerical simulations, requires the determination of the emission spectra and of the radiative losses due to free-free emission from the corresponding temperature-averaged and total Gaunt factors. Detailed calculati...

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Veröffentlicht in:	The Astrophysical journal. Supplement series 2017-09, Vol.232 (1), p.12
Hauptverfasser:	de Avillez, Miguel A., Breitschwerdt, Dieter
Format:	Artikel
Sprache:	eng
Schlagworte:	ASTROPHYSICS, COSMOLOGY AND ASTRONOMY atomic data atomic processes Boltzmann distribution BOLTZMANN STATISTICS Computer simulation COMPUTERIZED SIMULATION ELECTRONS EMISSION SPECTRA EQUILIBRIUM Equilibrium conditions EVOLUTION HELIUM IONS IONIZATION IRON IONS ISM: general MAGNESIUM IONS NEON IONS Numerical simulations Parameters PHOTONS PLASMA plasmas radiation mechanisms: general RADIATIVE COOLING radio continuum: general RELATIVISTIC RANGE SILICON IONS Temperature Thermal evolution Thermal plasmas
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