| Texto completo | |
| Autor(es): |
de Souza, Vitor
;
Biermman, Peter L. S.
;
Corbett, IF
Número total de Autores: 3
|
| Tipo de documento: | Artigo Científico |
| Fonte: | COSMIC MAGNETIC FIELDS: FROM PLANETS, TO STARS AND GALAXIES; v. 15, p. 3-pg., 2010-01-01. |
| Resumo | |
in this paper we briefly discuss the present status of the cosmic ray astrophysics under the light of the new data from the Pierre Auger Observatory. The measured energy spectrum is used to test the scenario of production in nearby radio galaxies. Within this framework the AGN correlation would require that most of the cosmic rays are heavy nuclei and are widely scattered by intergalactic magnetic fields. (AU) | |
| Processo FAPESP: | 08/04259-0 - Raios cósmicos de altas energias |
| Beneficiário: | Luiz Vitor de Souza Filho |
| Modalidade de apoio: | Auxílio à Pesquisa - Jovens Pesquisadores |