TY  - JOUR
AU  - Miceli, M.
AU  - Orlando, S.
AU  - Pereira Blanco, Victor
AU  - Acero, F.
AU  - Katsuda, S.
AU  - Decourchelle, A.
AU  - Winkler, F.P.
AU  - Bonito, R.
AU  - Reale, F.
AU  - Peres, G.
AU  - Li, J.
AU  - Dubner, G.
PY  - 2016
DO  - 10.1051/0004-6361/201628725
SN  - 1432-0746
UR  - https://hdl.handle.net/20.500.14352/19126
T2  - Astronomy & Astrophysics
AB  - Context. The supernova remnant SN 1006 is a source of high-energy particles and its southwestern limb is interacting with a dense ambient cloud, thus being a promising region for γ−ray hadronic emission.Aims. We aim at describing the physics and the...
LA  - eng
PB  - EDP Sciencies
KW  - Magnetic-field amplification
KW  - Nonlinear particle-acceleration
KW  - Supernova-remnants
KW  - Northeastern limb
KW  - Proper motions
KW  - Sn-1006
KW  - Ejecta
KW  - Energy
KW  - Simulations
KW  - Evolution
TI  - Modeling the shock-cloud interaction in SN 1006: unveiling the origin of nonthermal X-ray and gamma-ray emission
TY  - journal article
VL  - 593
ER  -