Imprints of mass accretion on properties of galaxy clusters

Monthly Notices of the Royal Astronomical Society

Volumn 362, Issue 3, 2005, Pages 1099-1108

  Faltenbacher, Andreas ^a,e   Allgood, Brandon ^b   Gottlöber, Stefan ^c   Yepes, Gustavo ^d   Hoffman, Yehuda ^e  

^a University of California at Santa Cruz   (United States)

^b UNIVERSITY OF CALIFORNIA   (United States)

^c ASTROPHYSIKALISCHES INSTITUT POTSDAM   (Germany)

^d UNIVERSIDAD AUTÓNOMA DE MADRID   (Spain)

^e HEBREW UNIVERSITY OF JERUSALEM   (Israel)

Author keywords

Galaxies: clusters: general; Large scale structure of Universe; Methods: numerical; Methods: statistical

Indexed keywords

GALAXIES; HYDRODYNAMICS; MERGING; NUMERICAL METHODS;

GALAXIES CLUSTERS; GALAXIES: CLUSTERS: GENERAL; LARGE SCALE STRUCTURE OF UNIVERSE; LARGE-SCALES; LONG RANGE CORRELATIONS; METHOD: NUMERICAL; METHODS:STATISTICAL; N-BODY SIMULATION; PROPERTY; SMOOTHED PARTICLE HYDRODYNAMICS;

ANGULAR MOMENTUM;

EID: 25144460606     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2005.09386.x     Document Type: Review

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