Relativistic electrons in the intracluster space of clusters of galaxies - The hard X-ray spectra and heating of the gas

Details Relativistic electrons in the intracluster space of clusters of galaxies - The hard X-ray spectra and heating of the gas Relativistic electrons in the intracluster space of clusters of galaxies - The hard X-ray spectra and heating of the gas

Jan 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979apj...227..364r&link_type=abstract

Astrophysical Journal, Part 1, vol. 227, Jan. 15, 1979, p. 364-369.

Astronomy and Astrophysics

Astrophysics

117

Energy Dissipation, Galactic Clusters, Gas Heating, High Energy Electrons, Intergalactic Media, X Ray Spectra, Energy Spectra, Magnetohydrodynamic Waves, Relativistic Particles

Scientific paper

An appropriate form for the steady-state intracluster relativistic electron energy spectrum is derived, taking into account all the dominant energy loss mechanisms. The Compton X-ray flux is calculated and compared with the soft X-ray thermal flux. The amount of heating of the intracluster gas by energy loss of relativistic electrons in electronic and Alfven wave excitations is estimated.

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