How does gas cool in dark matter haloes?

Monthly Notices of the Royal Astronomical Society

Volumn 383, Issue 2, 2008, Pages 777-790

  Viola, M ^a   Monaco, P ^a,b   Borgani, S ^a,b,c   Murante, G ^d   Tornatore, L ^a,e  

^a UNIVERSITY OF TRIESTE   (Italy)

^b INAF OSSERVATORIO ASTRONOMICO DI TRIESTE   (Italy)

^c SEZIONE DI TRIESTE   (Italy)

^d OSSERVATORIO ASTRONOMICO DI TORINO   (Italy)

^e SISSA   (Italy)

Author keywords

Cooling flows; Cosmology: theory; Methods: numerical

Indexed keywords

COOLING; DENSITY OF GASES; GALAXIES; GASES; NUMERICAL METHODS; SHELLS (STRUCTURES); TEMPERATURE;

CLASSICAL MODELING; COOLING FLOWS; COOLING MODEL; COOLING TIME; COSMOLOGY: THEORY; DARK MATTER HALOS; INITIAL CONDITIONS; METHOD: NUMERICAL; MORGANA; SMOOTHED PARTICLE HYDRODYNAMICS;

HYDRODYNAMICS;

EID: 37849050715     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2007.12598.x     Document Type: Article

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