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Non-Thermal Activity and Particle Acceleration in Clusters of Galaxies
2005
Highlights of Astronomy
AbstractEvidence for non-thermal activity in clusters of galaxies is well established from radio observations of synchrotron emission by relativistic electrons, and new windows (in EUV and Hard X-ray ranges) have provided more powerful tools for its investigation. The hard X-ray observations, notably from Coma, are summarized and results of a new RXTE observations of a high red-shift cluster are presented. It is shown that the most likely emission mechanism for these radiations is the inverse
doi:10.1017/s1539299600015872
fatcat:2xkdlop7zzaa5ae6v4ulkg4fiy