Hot and cooled baryons in smoothed particle hydrodynamic simulations of galaxy clusters: Physics and numerics

Monthly Notices of the Royal Astronomical Society

Volumn 367, Issue 4, 2006, Pages 1641-1654

  Borgani, S ^a,b,j   Dolag, K ^c   Murante, G ^a,d   Cheng, L M ^e   Springel, V ^c   Diaferio, A ^f   Moscardini, L ^g   Tormen, G ^h   Tornatore, L ^b,i   Tozzi, P ^b,j  

^a UNIVERSITY OF TRIESTE   (Italy)

^b SEZIONE DI TRIESTE   (Italy)

^c MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

^d OSSERVATORIO ASTRONOMICO DI TORINO   (Italy)

^e INSTITUTE OF THEORETICAL PHYSICS   (China)

^f UNIVERSITY OF TURIN   (Italy)

^g UNIVERSITY OF BOLOGNA   (Italy)

^h UNIVERSITY OF PADOVA   (Italy)

ⁱ SISSA   (Italy)

^j INAF OSSERVATORIO ASTRONOMICO DI TRIESTE   (Italy)

more..

Author keywords

Galaxies: clusters: general; Hydrodynamics

Indexed keywords

DENSITY OF GASES; GALAXIES; GASES; GRAVITATION; HADRONS; STARS; THERMODYNAMIC PROPERTIES;

CLUSTER OF GALAXIES; CLUSTER PHYSICS; DARK MATTER; GALAXIES CLUSTERS; GALAXIES: CLUSTERS: GENERAL; GAS PARTICLES; HYDRODYNAMIC SIMULATION; MASS RESOLUTION; SMOOTHED PARTICLE HYDRODYNAMICS; STARS FORMATION;

HYDRODYNAMICS;

EID: 33645664837     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2006.10075.x     Document Type: Article

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