Probing the dark matter profile of hot clusters and the M-T relation with XMM-Newton

Advances in Space Research

Volumn 36, Issue 4, 2005, Pages 659-662

  Pointecouteau, E ^a,c   Arnaud, M ^a   Pratt, G W ^b  

^a UNIVERSITÉ PARIS DIDEROT   (France)

^b MAX PLANCK INSTITUT FÜR EXTRATERRESTRISCHE PHYSIK   (Germany)

^c UNIVERSITY OF OXFORD   (United Kingdom)

Author keywords

Clusters of galaxies; Large scale structure; X rays; XMM Newton observations

Indexed keywords

COMPUTER SIMULATION; HIERARCHICAL SYSTEMS; SPACE RESEARCH; TEMPERATURE MEASUREMENT; X RAYS;

CLUSTERS OF GALAXIES; DARK MATTER; LARGE SCALE STRUCTURE; XMM-NEWTON OBSERVATIONS;

GALAXIES;

EID: 27744575906     PISSN: 02731177     EISSN: None     Source Type: Journal    
DOI: 10.1016/j.asr.2005.02.016     Document Type: Conference Paper

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