Comparing the temperatures of galaxy clusters from hydrodynamical N-body simulations to Chandra and XMM-Newton observations

Monthly Notices of the Royal Astronomical Society

Volumn 354, Issue 1, 2004, Pages 10-24

  Mazzotta, P ^a,b   Rasia, E ^c   Moscardini, L ^d   Tormen, G ^c  

^a UNIVERSITY OF ROME TOR VERGATA   (Italy)

^b HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^c UNIVERSITY OF PADOVA   (Italy)

^d UNIVERSITY OF BOLOGNA   (Italy)

Author keywords

Cosmology: theory; Galaxies: clusters: general; Galaxies: general; Hydrodynamics; Methods: numerical; X rays: general

Indexed keywords

COSMOLOGY; GALAXIES; NUMERICAL METHODS; NUMERICAL MODELS; SPECTROSCOPIC ANALYSIS;

CHANDRA; COSMOLOGY: THEORY; GALAXIES CLUSTERS; GALAXIES GENERAL; GALAXIES: CLUSTERS: GENERAL; METHOD: NUMERICAL; N-BODY SIMULATION; SHOCK FRONTS; X-RAY GENERAL; X-RAY OBSERVATIONS;

SHOCK WAVES;

EID: 7544247231     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2004.08167.x     Document Type: Article

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