Suzaku Observations of Non-thermal X-ray Emission from Galaxy Clusters

Details Suzaku Observations of Non-thermal X-ray Emission from Galaxy Clusters Suzaku Observations of Non-thermal X-ray Emission from Galaxy Clusters

Jul 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aipc..921..488k&link_type=abstract

THE FIRST GLAST SYMPOSIUM. AIP Conference Proceedings, Volume 921, pp. 488-489 (2007).

Physics

Galaxy Clusters, X-Ray, Gamma-Ray

Scientific paper

Clusters of galaxies are the largest gravitationally-bound system in the universe, and possible candidates of particle accelerator. The detection of diffuse radio emission, which is synchrotron emission caused by relativistic electrons, supports the scenario. The direct measurements by X-ray/Gamma-ray are important to clarify the non-thermal view of clusters. We present the initial hard X-ray research of galaxy clusters (especially for A3376) with Suzaku, which has excellent sensitivity in a few tens keV. GLAST will make X-ray results be more valuable to discuss particle acceleration in galaxy clusters.

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