Radiation Properties of High-Energy Astrophysical Plasmas

Details Radiation Properties of High-Energy Astrophysical Plasmas Radiation Properties of High-Energy Astrophysical Plasmas

Jul 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005ap%26ss.298..155m&link_type=abstract

Astrophysics and Space Science, Volume 298, Issue 1-2, pp. 155-162

Astronomy and Astrophysics

Astrophysics

Radiation Mechanisms, X-Rays, Supernova Remnants

Scientific paper

We discuss radiation properties of plasmas in high-energy astrophysics with a keyword nonequilibrium: non-LTE level populations, nonequilibrium ionization, and non-Maxwellian distribution function, beginning with radiative transfer. We focus particularly on supernova remnants interacting with the circumstellar/interstellar matter, and also mention line emission processes in accretion gas onto a neutron star or black hole, and in the X-ray afterglow of γ-ray bursts.

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