Massive and refined: II. the statistical properties of turbulent motions in massive galaxy clusters with high spatial resolution

Astronomy and Astrophysics

Volumn 529, Issue , 2011, Pages

  Vazza, F ^a,b   Brunetti, G ^b   Gheller, C ^c   Brunino, R ^c   Bruggen M ^a  

^a JACOBS UNIVERSITY BREMEN   (Germany)

^b INAF ISTITUTO DI RADIOASTRONOMIA   (Italy)

^c CINECA   (Italy)

Author keywords

galaxies: clusters: general; large scale structure of Universe; methods: numerical

Indexed keywords

ADAPTIVE MESH REFINEMENT CODES; CHAOTIC MOTIONS; DYNAMICAL STATE; GALAXIES: CLUSTERS: GENERAL; GALAXY CLUSTERS; HIGH SPATIAL RESOLUTION; INTRA-CLUSTER MEDIUM; LARGE SCALE STRUCTURE OF UNIVERSE; METHODS: NUMERICAL; RADIO HALO; RELATIVISTIC PARTICLES; SEMI-ANALYTICAL; SPATIAL PROPERTIES; SPATIAL SCALE; STATISTICAL PROPERTIES; TURBULENT KINETIC ENERGY; TURBULENT MOTION; XMM-NEWTON;

GALAXIES; KINETIC ENERGY; NUMERICAL METHODS; REYNOLDS NUMBER; TURBULENCE;

MERGING;

EID: 79952945896     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201016015     Document Type: Article

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