Interaction of high-energy particles with intergalactic gas

Details Interaction of high-energy particles with intergalactic gas Interaction of high-energy particles with intergalactic gas

Jul 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984afz....21..103s&link_type=abstract

(Astrofizika, vol. 21, July-Aug. 1984, p. 103-109) Astrophysics (ISSN 0571-7132), vol. 20, no. 4, Jan. 1985, p. 415-418. Transla

Astronomy and Astrophysics

Astronomy

Cosmic Rays, Electron Scattering, Galactic Clusters, High Energy Interactions, Intergalactic Media, Plasma Heating, Electron Gas, Heao 2, High Energy Electrons, Maxwell-Boltzmann Density Function, Velocity Distribution, X Ray Astronomy

Scientific paper

It is shown that the energy of cosmic rays supplied to the intergalactic medium from galaxies is an effective source of its heating. Under the conditions of the intergalactic medium, a non-Maxwellian distribution of the electron gas can be formed with the 'tail' of the distribution cut off. The interaction of the electrons with the cosmic rays cannot sustain the tail. The X-ray spectrum of the gas in the cluster A 2142 appears to reflect the deviation from the Maxwellian distribution.

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