Radial temperature profiles for a large sample of galaxy clusters observed with XMM-Newton

Astronomy and Astrophysics

Volumn 486, Issue 2, 2008, Pages 359-373

  Leccardi, A ^a,b   Molendi, S ^b  

^a UNIVERSITY OF MILAN   (Italy)

^b INAF IASF MILANO   (Italy)

Author keywords

Cosmology: observations; Galaxies: clusters: general; X rays: galaxies: clusters

Indexed keywords

EMISSION SPECTROSCOPY; FLUID DYNAMICS; FLUID MECHANICS; GALAXIES; REUSABILITY; TEMPERATURE CONTROL;

BACKGROUND MODELING; BACKGROUND SUBTRACTION; CLUSTER TEMPERATURES; EXTENSIVE SIMULATIONS; GALAXY CLUSTERING; HYDRODYNAMIC SIMULATIONS; LARGE SAMPLE; MEAN TEMPERATURES; RADIAL TEMPERATURE PROFILES; RED SHIFTING; SIMULATED SPECTRUM; SPECTRAL COMPONENTS; SYSTEMATIC (CO); SYSTEMATIC EFFECTS; SYSTEMATIC UNCERTAINTIES; TEMPERATURE PROFILING; X-RAY EXPERIMENTS; XMM-NEWTON;

SYSTEMATIC ERRORS;

EID: 47249093188     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:200809538     Document Type: Article

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