Modelling shock heating in cluster mergers - I. Moving beyond the spherical accretion model

Monthly Notices of the Royal Astronomical Society

Volumn 376, Issue 2, 2007, Pages 497-522

  McCarthy, I G ^a   Bower, R G ^a   Balogh, M L ^b   Voit, G M ^c   Pearce, F R ^d   Theuns, T ^a,e   Babul, A ^f   Lacey, C G ^a   Frenk, C S ^a  

^a DURHAM UNIVERSITY   (United Kingdom)

^b UNIVERSITY OF WATERLOO   (Canada)

^c MICHIGAN STATE UNIVERSITY   (United States)

^d UNIVERSITY OF NOTTINGHAM   (United Kingdom)

^e UNIVERSITY OF ANTWERP   (Belgium)

^f UNIVERSITY OF VICTORIA   (Canada)

Author keywords

Cosmology: theory; Galaxies: clusters: general; Galaxies: formation

Indexed keywords

ANALYTICAL MODELS; COSMOLOGY; GALAXIES; GASES; GRAVITATION; HEATING; KINETIC ENERGY; KINETICS; SHOCK WAVES;

COSMOLOGY: THEORY; DENSITY STRUCTURES; ENERGY; ENTROPY GENERATION; GALAXIES: CLUSTERS: GENERAL; GALAXY FORMATIONS; INTRACLUSTER MEDIUM; MASS RATIO; PHYSICAL PROCESS; TEMPERATURE STRUCTURE;

ENTROPY;

EID: 34247183236     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2007.11465.x     Document Type: Article

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