Turbulent motions and shocks waves in galaxy clusters simulated with adaptive mesh refinement

Astronomy and Astrophysics

Volumn 504, Issue 1, 2009, Pages 33-43

  Vazza, F ^a,b   Brunetti, G ^b   Kritsuk, A ^c   Wagner, R ^c,d   Gheller, C ^e   Norman, M ^c,d  

^a UNIVERSITY OF BOLOGNA   (Italy)

^b INAF ISTITUTO DI RADIOASTRONOMIA   (Italy)

^c UNIVERSITY OF CALIFORNIA   (United States)

^d UNIVERSITY OF CALIFORNIA   (United States)

^e CINECA   (Italy)

Author keywords

Galaxies: Clusters: General; Intergalactic medium; Large scale structure of Universe; Methods: Numerical

Indexed keywords

ADAPTIVE MESH REFINEMENT; CHAOTIC MOTIONS; GALAXIES: CLUSTERS: GENERAL; GALAXY CLUSTERS; GAS VELOCITY; HIERARCHICAL ASSEMBLIES; INTERGALACTIC MEDIUM; LARGE-SCALE STRUCTURE OF UNIVERSE; METHODS: NUMERICAL; SPATIAL RESOLUTION; SPECTRAL PROPERTIES; TIME EVOLUTIONS; TURBULENT EDDY; TURBULENT MOTION; VELOCITY FIELD;

COSMOLOGY; IMAGE RESOLUTION; NUMERICAL METHODS;

GALAXIES;

EID: 70149101751     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200912535     Document Type: Article

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