Cosmic Rays and Non-Thermal Emission in Galaxy Clusters
| dc.creator | Colafrancesco, S. | |
| dc.date | 1999-07-23 | |
| dc.date.accessioned | 2026-07-07T02:32:37Z | |
| dc.date.available | 2026-07-07T02:32:37Z | |
| dc.description | We discuss the origin of thermal and non-thermal phenomena in galaxy clusters. Specifically, we present some expectations for the non-thermal emission (from radio to gamma ray wavelenghts) expected in a model in which secondary electrons are produced via $pp$ collisions in the intracluster medium. We also discuss the possibility to test this cosmic ray model in the light of recent data on radio halos and hard X-ray excesses found in nearby galaxy clusters. | |
| dc.description | 6 pages, 4 Figures, to appear in proceedings of the Ringberg workshop on "Diffuse Thermal and Relativistic Plasma in Galaxy Clusters", April 1999, H. Boehringer, L. Feretti, P. Schuecker (eds.) | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9907329 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9907329 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/14527 | |
| dc.subject | Astrophysics | |
| dc.title | Cosmic Rays and Non-Thermal Emission in Galaxy Clusters | |
| dc.type | text |