GALACTIC AND EXTRAGALACTIC SUPERNOVA REMNANTS AS SITES OF PARTICLE ACCELERATION
| dc.contributor.author | Sasaki, Manami | |
| dc.date.accessioned | 2021-12-01T13:23:15Z | |
| dc.date.available | 2021-12-01T13:23:15Z | |
| dc.date.issued | 2013 | |
| dc.identifier.citation | Acta Polytechnica. 2013, vol. 53, no. A, p. 612-616. | |
| dc.identifier.issn | 1210-2709 (print) | |
| dc.identifier.issn | 1805-2363 (online) | |
| dc.identifier.uri | http://hdl.handle.net/10467/98656 | |
| dc.description.abstract | Supernova remnants, owing to their strong shock waves, are likely sources of Galactic cosmic rays. Studies of supernova remnants in X-rays and gamma rays provide us with new insights into the acceleration of particles to high energies. This paper reviews the basic physics of supernova remnant shocks and associated particle acceleration and radiation processes. In addition, the study of supernova remnant populations in nearby galaxies and the implications for Galactic cosmic ray distribution are discussed. | en |
| dc.format.mimetype | application/pdf | |
| dc.language.iso | eng | |
| dc.publisher | České vysoké učení technické v Praze | cs |
| dc.publisher | Czech Technical University in Prague | en |
| dc.relation.ispartofseries | Acta Polytechnica | |
| dc.relation.uri | https://ojs.cvut.cz/ojs/index.php/ap/article/view/1918 | |
| dc.rights | Creative Commons Attribution 4.0 International License | en |
| dc.rights.uri | http://creativecommons.org/licenses/by/4.0/ | |
| dc.title | GALACTIC AND EXTRAGALACTIC SUPERNOVA REMNANTS AS SITES OF PARTICLE ACCELERATION | |
| dc.type | article | en |
| dc.date.updated | 2021-12-01T13:23:15Z | |
| dc.identifier.doi | 10.14311/AP.2013.53.0612 | |
| dc.rights.access | openAccess | |
| dc.type.status | Peer-reviewed | |
| dc.type.version | publishedVersion |
Soubory tohoto záznamu
Tento záznam se objevuje v následujících kolekcích
Kromě případů, kde je uvedeno jinak, licence tohoto záznamu je Creative Commons Attribution 4.0 International License