3D simulations of supernova remnants evolution including non-linear particle acceleration

Astronomy and Astrophysics

Volumn 509, Issue 1, 2010, Pages

  Ferrand, G ^a   Decourchelle, A ^a   Ballet, J ^a   Teyssier, R ^a,b   Fraschetti, F ^c,d  

^a CNRS   (France)

^b UNIVERSITY OF ZURICH   (Switzerland)

^c UNIVERSITÉ PARIS DIDEROT   (France)

^d University of Arizona   (United States)

Author keywords

ISM; Numerical; Supernova remnants Instabilities Cosmic rays Acceleration of particles Methods

Indexed keywords

ACCELERATION; ASTRONOMY; COSMIC RAYS; COSMOLOGY; FLUID DYNAMICS; HYDRODYNAMICS; NUMERICAL METHODS; PARTICLE ACCELERATOR ACCESSORIES; PARTICLE ACCELERATORS; THREE DIMENSIONAL COMPUTER GRAPHICS;

3D SIMULATIONS; ACCELERATED PARTICLES; ACCELERATION OF PARTICLES; ADIABATIC INDICES; BACK REACTION; CHANDRA; CONTACT DISCONTINUITIES; DENSITY PROFILE; ENERGETIC PARTICLES; GALACTIC COSMIC RAYS; HYDRODYNAMIC CODES; HYDRODYNAMIC INSTABILITIES; INJECTION LEVELS; INJECTION RATES; ISM; KINETIC MODELS; MORPHOLOGICAL EVOLUTION; NON-LINEAR; RAYLEIGH-TAYLOR; SEMI-ANALYTICAL; SHOCK ACCELERATION; SUPERNOVA REMNANTS; TIME-DEPENDENT COMPRESSION; UNSTABLE REGIONS; X RAY SATELLITES; XMM-NEWTON;

THREE DIMENSIONAL;

EID: 76349110988     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200913666     Document Type: Article

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