Non thermal emission in clusters of galaxies
| dc.creator | Arnaud, M. | |
| dc.date | 2008-01-24 | |
| dc.date.accessioned | 2026-07-07T08:56:14Z | |
| dc.date.available | 2026-07-07T08:56:14Z | |
| dc.description | I briefly review our current knowledge of the non thermal emission from galaxy clusters and discuss future prospect with Simbol-X. Simbol-X will map the hard X-ray emission in clusters, determine its origin and disentangle the thermal and non-thermal components. Correlated with radio observations, the observation of the non-thermal X-ray emission, when confirmed, will allow to map both the magnetic field and the relativistic electron properties, key information to understand the origin and acceleration of relativistic particles in clusters and its impact on cluster evolution. | |
| dc.description | 6 pages, 7 figures, invited talk at the International Workshop, "Simbol X: The Hard X-ray Universe in Focus", held in Bologna 14-16 May 2007. To be published in Memorie della Societa' Astronomica Italiana | |
| dc.identifier | https://arxiv.org/abs/0801.3814 | |
| dc.identifier | http://arxiv.org/abs/0801.3814 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/146539 | |
| dc.subject | Astrophysics | |
| dc.title | Non thermal emission in clusters of galaxies | |
| dc.type | text |