TY  - JOUR
AU  - Barrio Uña, Juan Abel
AU  - Contreras González, José Luis
AU  - Fonseca González, María Victoria
AU  - Hoang, Kim Dinh
AU  - López Moya, Marcos
AU  - Miener, Tjark
AU  - Morcuende, D.
AU  - Peñil Del Campo, Pablo
AU  - Saha, Lab
PY  - 2023
DO  - 10.1051/0004-6361/202038748
SN  - 0004-6361
UR  - https://hdl.handle.net/20.500.14352/72202
T2  - Astronomy & Astrophysics
AB  - Context. Diffusive shock acceleration (DSA) is the most promising mechanism that accelerates Galactic cosmic rays (CRs) in the shocks of supernova remnants (SNRs). It is based on particles scattering caused by turbulence ahead and behind the shock....
LA  - eng
PB  - EDP Sciencies
KW  - Large-area telescope
KW  - Diffusive shock acceleration
KW  - Magnetic-field amplification
KW  - Supernova remnant g78.2+2.1
KW  - X-ray
KW  - Streaming instability
KW  - Likelihood analysis
KW  - Psr j2021+4026
KW  - Emission
KW  - Region
TI  - Study of the GeV to TeV morphology of the gamma Cygni SNR (G 78.2+2.1) with MAGIC and Fermi-LAT: Evidence for cosmic ray escape
TY  - journal article
VL  - 670
ER  -