Substructure of the galaxy clusters in the REXCESS sample: Observed statistics and comparison to numerical simulations

Astronomy and Astrophysics

Volumn 514, Issue 3, 2010, Pages

  Bohringer H ^a   Pratt, G W ^a,b   Arnaud, M ^b   Borgani, S ^c   Croston, J H ^d   Ponman, T J ^e   Ameglio, S ^c,f   Temple, R F ^e   Dolag, K ^g  

^a MAX PLANCK INSTITUT FÜR EXTRATERRESTRISCHE PHYSIK   (Germany)

^b CEA SACLAY   (France)

^c UNIVERSITY OF TRIESTE   (Italy)

^d UNIVERSITY OF SOUTHAMPTON   (United Kingdom)

^e UNIVERSITY OF BIRMINGHAM   (United Kingdom)

^f UNIVERSITY OF SOUTHERN CALIFORNIA   (United States)

^g MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

Author keywords

Cosmology: observations; Galaxies: clusters: intracluster medium; X rays: galaxies: clusters

Indexed keywords

COMPUTER SIMULATION; COSMOLOGY; LUMINANCE; MONTE CARLO METHODS; MORPHOLOGY; REGRESSION ANALYSIS; STATISTICAL MECHANICS;

ALL-SKY; BULK PROPERTIES; CHARACTERISATION; CLUSTER FORMATIONS; CLUSTER MASS; CLUSTER MORPHOLOGY; CLUSTER SURVEY; COSMOLOGY: OBSERVATION; DYNAMIC RANGE; DYNAMICAL STATE; GALAXY CLUSTERS; INTRA-CLUSTER MEDIUM; LARGE CLUSTERS; NUMERICAL SIMULATION; PHYSICAL PROCESS; POWER RATIO; PROJECTION EFFECTS; RED SHIFT; REPRESENTATIVE SAMPLE; SHIFT PARAMETERS; STATISTICAL TOOLS; SUBSTRUCTURE PARAMETER; VIEWING ANGLE; WEAK CORRELATION; X RAYS: GALAXIES: CLUSTERS; X-RAY LUMINOSITY; XMM-NEWTON;

GALAXIES;

EID: 77952051949     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200913911     Document Type: Article

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