The formation of entropy cores in non-radiative galaxy cluster simulations: Smoothed particle hydrodynamics versus adaptive mesh refinement

Monthly Notices of the Royal Astronomical Society

Volumn 440, Issue 4, 2014, Pages 3243-3256

  Power, C ^a   Read, J I ^b   Hobbs, A ^c  

^a UNIVERSITY OF WESTERN AUSTRALIA   (Australia)

^b UNIVERSITY OF SURREY   (United Kingdom)

^c ETH ZURICH   (Switzerland)

Author keywords

Cosmology: theory; Galaxies: clusters: intracluster medium; Large scale structure of universe; Methods: numerical

Indexed keywords

COSMOLOGY; GALAXIES; HYDRODYNAMICS; MESH GENERATION; NUMERICAL ANALYSIS; NUMERICAL METHODS;

ADAPTIVE MESH REFINEMENT; CLUSTER ASSEMBLY; CLUSTER SIMULATIONS; COSMOLOGY: THEORY; GALAXIES CLUSTERS; GALAXIES: CLUSTERS: INTRACLUSTER MEDIUMS; LARGE SCALE STRUCTURE OF UNIVERSE; METHOD: NUMERICAL; NON-RADIATIVE; SMOOTHED PARTICLE HYDRODYNAMICS;

ENTROPY;

EID: 84899889636     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1093/mnras/stu418     Document Type: Article

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