Shapes of clusters and groups of galaxies: Comparison of model predictions with observations

Monthly Notices of the Royal Astronomical Society

Volumn 366, Issue 4, 2006, Pages 1503-1510

  Paz, D J ^a,b   Lambas, D G ^a,b   Padilla, N ^c   Merchan M ^a,b  

^a Instituto de Astronomia Teorica y Experimental   (Argentina)

^b Facultad de Ciencias Naturales e Instituto M Lillo   (Argentina)

^c PONTIFICIA UNIVERSIDAD CATÓLICA DE CHILE   (Chile)

Author keywords

Cosmology: theory; Galaxies: kinematics and dynamics; Large scale structure of Universe; Methods: N body simulations

Indexed keywords

SOLVENTS; SURVEYS;

COMPARISON OF MODELS; COSMOLOGY: THEORY; GALAXIES: KINEMATICS AND DYNAMICS; GALAXY GROUP; GROUP MEMBERS; LARGE SCALE STRUCTURE OF UNIVERSE; METHODS:N-BODY SIMULATIONS; MODEL PREDICTION; PROPERTY; THREE-DIMENSIONAL SHAPE;

GALAXIES;

EID: 33644590889     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2005.09934.x     Document Type: Article

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