Synchrotron and inverse Compton processes in X-ray clusters of galaxies

Details Synchrotron and inverse Compton processes in X-ray clusters of galaxies Synchrotron and inverse Compton processes in X-ray clusters of galaxies

Oct 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975pasau...2..327v&link_type=abstract

(Astronomical Society of Australia, Annual General Meeting, 9th, Parkes, New South Wales, Australia, May 14-16, 1975.) Astronomi

Astronomy and Astrophysics

Astronomy

3

Bremsstrahlung, Compton Effect, Galactic Clusters, Synchrotron Radiation, X Ray Sources, Extragalactic Radio Sources, Microwave Emission, Spaceborne Astronomy, Uhuru Satellite

Scientific paper

The extended nature of the X-ray source is one of the best criteria for identifying a cluster of galaxies with an X-ray source. Mechanisms for X-ray emission from an intracluster medium are considered, taking into account thermal bremsstrahlung and the Compton scattering of photons from the microwave background to X-ray energies by relativistic electrons. A quantitative link between the synchrotron and inverse Compton processes in the intracluster medium is presented.

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