HAL : in2p3-00461069, version 1
 arXiv : 1001.1419
 Astrophysical Journal Letters 710 (2010) L92-L97
 Fermi-LAT discovery of GeV gamma-ray emission from the young supernova remnant Cassiopeia A
 Fermi-LAT Collaboration(s)
 (10/02/2010)
 We report on the first detection of GeV high-energy gamma-ray emission from a young supernova remnant with the Large Area Telescope aboard the Fermi Gamma-ray Space Telescope. These observations reveal a source with no discernible spatial extension detected at a significance level of 12.2$\sigma$ above 500 MeV at a location that is consistent with the position of the remnant of the supernova explosion that occurred around 1680 in the Cassiopeia constellation - Cassiopeia A. The gamma-ray flux and spectral shape of the source are consistent with a scenario in which the gamma-ray emission originates from relativistic particles accelerated in the shell of this remnant. The total content of cosmic rays (electrons and protons) accelerated in Cas A can be estimated as $W_{\mathrm{CR}} \approx (1-4) \times 10^{49}$ erg thanks to the well-known density in the remnant assuming that the observed gamma-ray originates in the SNR shell(s). The magnetic field in the radio-emitting plasma can be robustly constrained as B $\gt 0.1$ mG, providing new evidence of the magnetic field amplification at the forward shock and the strong field in the shocked ejecta.
 Thème(s) : Physique/Astrophysique/Phénomènes cosmiques de haute energiePlanète et Univers/Astrophysique/Phénomènes cosmiques de haute energie
 Mot(s)-clé(s) : acceleration of particles – ISM: individual objects (Cassiopeia A) – radiation mechanisms: non-thermal
 Lien vers le texte intégral : http://fr.arXiv.org/abs/1001.1419
 in2p3-00461069, version 1 http://hal.in2p3.fr/in2p3-00461069 oai:hal.in2p3.fr:in2p3-00461069 Contributeur : Virginie Mas <> Déposé pour le compte de : David Smith <> Soumis le : Mercredi 3 Mars 2010, 11:38:12 Dernière modification le : Jeudi 4 Mars 2010, 10:15:56