Dynamical difference between the cD galaxy and the diffuse, stellar component in simulated galaxy clusters

Monthly Notices of the Royal Astronomical Society

Volumn 405, Issue 3, 2010, Pages 1544-1559

  Dolag, K ^a   Murante, G ^b   Borgani, S ^c,d,e  

^a MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

^b OSSERVATORIO ASTRONOMICO DI TORINO   (Italy)

^c UNIVERSITY OF TRIESTE   (Italy)

^d SEZIONE DI TRIESTE   (Italy)

^e INAF OSSERVATORIO ASTRONOMICO DI TRIESTE   (Italy)

Author keywords

Cosmology: theory; Galaxies: cluster: general; Galaxies: evolution; Hydrodynamics; Methods: numerical

Indexed keywords

COSMOLOGY; FLUID DYNAMICS; GALAXIES; NUMERICAL METHODS; VELOCITY DISTRIBUTION;

COSMOLOGY: THEORY; DIFFUSE COMPONENTS; GALAXIES CLUSTERS; GALAXIES: CLUSTERS: GENERAL; GALAXY EVOLUTION; METHOD: NUMERICAL; STELLAR POPULATIONS; STELLARS; TWO-COMPONENT; WITHIN CLUSTERS;

STARS;

EID: 77954902708     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2010.16583.x     Document Type: Article

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