Evolution of the metal content of the intracluster medium with hydrodynamical simulations

Monthly Notices of the Royal Astronomical Society

Volumn 386, Issue 3, 2008, Pages 1265-1273

  Fabjan, D ^a,b,c   Tornatore, L ^a,b,c   Borgani, S ^a,b,c   Saro, A ^a,c   Dolag, K ^d  

^a UNIVERSITY OF TRIESTE   (Italy)

^b INAF OSSERVATORIO ASTRONOMICO DI TRIESTE   (Italy)

^c SEZIONE DI TRIESTE   (Italy)

^d MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

Author keywords

Cosmology: theory; Galaxies: abundances; Intergalactic medium; Methods: numerical; X rays: galaxies: clusters

Indexed keywords

COSMOLOGY; HYDRODYNAMICS; LOCKS (FASTENERS); METALS; NUMERICAL METHODS; SUPERNOVAE;

COSMOLOGY: THEORY; GALAXIES ABUNDANCES; INITIAL MASS; INTERGALACTIC MEDIUM; INTRACLUSTER MEDIUM; MASS FUNCTIONS; METALLICITIES; METHOD: NUMERICAL; STARS FORMATION; X-RAYS GALAXIES CLUSTERS;

GALAXIES;

EID: 43049129635     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2008.13122.x     Document Type: Article

References (60)