| Issue |
|
EAS Publications Series
Volume 20,
2006
Mass Profiles and Shapes of Cosmological Structures
|
|
Page(s)
|
|
183 - 186 |
| DOI |
|
10.1051/eas:2006068 |
| Published online |
|
19 May 2006 |
|
Mass Profiles and Shapes of Cosmological Structures
G.A. Mamon, F. Combes, C. Deffayet and B. Fort (eds)
EAS Publications Series, 20 (2006) 183-186DOI: 10.1051/eas:2006068
Relaxed and unrelaxed clusters of galaxies seen in X-rays
F. Durret1, G.B. Lima Neto2, C. Adami3, J. Bagchi4, G. Covone5, W. Forman6, J.-P. Kneib3, E. Slezak7 and G. Soucail8 1
Institut d'Astrophysique de Paris, CNRS,
98bis Bd. Arago, 75014 Paris, France
2
IAG, São Paulo, Brazil
3
LAM, Marseille, France
4
IUCAA, Pune, India
5
INAF, Oss. Capodimonte, Naples, Italy
6
CfA, Cambridge MA, USA
7
OCA, Nice, France
8
OMP, Toulouse, France
Abstract
Recent X-ray observations have been showing that the old vision of
clusters as peacefully relaxed structures is in most cases absolutely
wrong. Coupled with optical and radio observations, these X-ray data
show evidence for violent mechanisms. Results based on XMM-Newton gas
temperature maps for four clusters will be presented here.
© EAS, EDP Sciences 2006
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