On the shape of the spectrum of cosmic rays accelerated inside superbubbles

Astronomy and Astrophysics

Volumn 510, Issue 1, 2010, Pages

  Ferrand, G ^a   Marcowith, A ^b  

^a CEA SACLAY   (France)

^b UNIVERSITÉ MONTPELLIER II   (France)

Author keywords

Acceleration of particles; Cosmic rays; ISM: supernova remnants; Shock waves; Turbulence

Indexed keywords

ACCELERATION OF PARTICLES; BUBBLE PARAMETERS; COLLECTIVE EFFECTS; DIMENSIONLESS PARAMETERS; ENERGETIC PARTICLES; FERMI 2; HIGH ENERGY PROTON; HIGH-ENERGY EMISSIONS; ISM: SUPERNOVA REMNANTS; LINEAR ACCELERATIONS; MAGNETIC TURBULENCE; MASSIVE STARS; MONTE CARLO SIMULATION; OB ASSOCIATION; PARTICLE ACCELERATION; PARTICLE SPECTRA; PROTON ENERGY LOSS; RE-ACCELERATION; SEMI-ANALYTICAL MODEL; SHOCK FRONTS; SUPERNOVA REMNANTS;

ACCELERATION; COMPUTER SIMULATION; COSMIC RAYS; COSMOLOGY; ENERGY DISSIPATION; HIGH ENERGY PHYSICS; MATHEMATICAL MODELS; MONTE CARLO METHODS; PARTICLE ACCELERATOR ACCESSORIES; PARTICLE ACCELERATORS; PROTONS; SHOCK WAVES; STARS; TURBULENCE;

ATMOSPHERIC OPTICS;

EID: 79952836481     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200913520     Document Type: Article

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