Equilibrium emission of low-density, optically thick plasma

Details Equilibrium emission of low-density, optically thick plasma Equilibrium emission of low-density, optically thick plasma

Feb 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984pazh...10...83n&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 10, Jan. 1984, p. 76-80) Soviet Astronomy Letters (ISSN 0360-0327), vol. 10, Jan.-Feb.

Astronomy and Astrophysics

Astronomy

1

Emission Spectra, Hydrogen Plasma, Plasma Spectra, Rarefied Plasmas, X Ray Sources, Astronomical Spectroscopy, Compton Effect, Luminosity, Nonrelativistic Mechanics, Optical Thickness

Scientific paper

The plasma emission spectrum and luminosity are calculated theoretically for an optically thick fully ionized nonrelativistic H plasma with an electron density sufficiently low that the primary mechanism not conserving the number of photons is double Compton scattering. The results are considered applicable to quasar or galaxy models with accretion disks having super-Eddington luminosity and gas pressure dominated by radiation pressure.

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