Simulation of the growth of the 3D Rayleigh-Taylor instability in supernova remnants using an expanding reference frame

Astronomy and Astrophysics

Volumn 515, Issue 11, 2010, Pages

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

^a UNIVERSITÉ PARIS DIDEROT   (France)

^b UNIVERSITÉ PARIS DIDEROT   (France)

^c The University of Arizona   (United States)

^d UNIVERSITY OF ZURICH   (Switzerland)

Author keywords

Acceleration of particles; Hydrodynamics; ISM: supernova remnants

Indexed keywords

ACCELERATION; COMPUTER SIMULATION; COSMOLOGY; FLUID DYNAMICS; HYDRODYNAMICS; IONIZING RADIATION; PARTICLE ACCELERATOR ACCESSORIES; PARTICLE ACCELERATORS; RAYLEIGH SCATTERING;

ACCELERATED PARTICLES; ACCELERATION OF PARTICLES; ADAPTIVE MESH REFINEMENT CODES; ADIABATIC INDICES; BLAST WAVES; CO-ORDINATE SYSTEM; CONTACT DISCONTINUITIES; EARLY GROWTH; FINGER-LIKE STRUCTURE; INTERSTELLAR MEDIUMS; ISM: SUPERNOVA REMNANTS; NUMERICAL DIFFUSION; NUMERICAL SIMULATION; PARTICLE ACCELERATION; RAYLEIGH-TAYLOR; RAYLEIGH-TAYLOR INSTABILITIES; REFERENCE FRAME; SELF-SIMILAR; SUPERNOVA REMNANTS;

ASTRONOMY;

EID: 77953628292     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200912692     Document Type: Article

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