Nonthermal Activity and Particle Acceleration in Clusters of Galaxies
| dc.creator | Petrosian, Vahe' | |
| dc.date | 2004-08-17 | |
| dc.date.accessioned | 2026-07-07T02:14:18Z | |
| dc.date.available | 2026-07-07T02:14:18Z | |
| dc.description | Evidence for nonthermal 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 redshift cluster are presented. It is shown that the most likely emission mechanisms for these radiations is the inverse Compton scattering of the cosmic microwave background photons by the same electrons responsible for the radio radiation. Various scenarios for acceleration of the electrons are considered and it is shown that the most likely model is episodic acceleration by shocks or turbulence, presumably induced by merger activity, of high energy electrons injected into the intercluster medium by galaxies or active galactic nuclei. | |
| dc.description | 5 pages. Presented at IAU General Assembly, Sydney, Australia | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0408317 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0408317 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/8064 | |
| dc.subject | Astrophysics | |
| dc.title | Nonthermal Activity and Particle Acceleration in Clusters of Galaxies | |
| dc.type | text |