Non-thermal physics of galaxy clusters

Details Non-thermal physics of galaxy clusters Non-thermal physics of galaxy clusters

Dec 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011sf2a.conf..111f&link_type=abstract

SF2A-2011: Proceedings of the Annual meeting of the French Society of Astronomy and Astrophysics Eds.: G. Alecian, K. Belkacem,

Astronomy and Astrophysics

Astrophysics

Galaxies: Clusters: General, Radio Continuum: Galaxies

Scientific paper

Deep radio observations of galaxy clusters have revealed the existence of diffuse radio sources related to the presence of relativistic electrons and weak magnetic fields in the intracluster volume. Non-thermal intracluster phenomena are reviewed, together with the importance for this research field of joint radio, mm, X- and Gamma-ray observations of galaxy clusters.

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