Hostname: page-component-6bf8c574d5-7jkgd Total loading time: 0 Render date: 2025-02-22T23:22:59.378Z Has data issue: false hasContentIssue false
  • English
  • Français

Relaxed and unrelaxed clusters of galaxies seen in X-rays

Published online by Cambridge University Press:  19 May 2006

G.A. Mamon ,
F. Combes ,
C. Deffayet ,
B. Fort ,
F. Durret ,
G.B. Lima Neto ,
C. Adami ,
J. Bagchi ,
G. Covone  and
W. Forman
...Show all authors
F. Durret
Affiliation:
Institut d'Astrophysique de Paris, CNRS, 98bis Bd. Arago, 75014 Paris, France
G.B. Lima Neto
Affiliation:
IAG, São Paulo, Brazil
C. Adami
Affiliation:
LAM, Marseille, France
J. Bagchi
Affiliation:
IUCAA, Pune, India
G. Covone
Affiliation:
INAF, Oss. Capodimonte, Naples, Italy
W. Forman
Affiliation:
CfA, Cambridge MA, USA
J.-P. Kneib
Affiliation:
LAM, Marseille, France
E. Slezak
Affiliation:
OCA, Nice, France
G. Soucail
Affiliation:
OMP, Toulouse, France
Get access

Abstract


Recent X-ray observations have been showing that the old vision ofclusters as peacefully relaxed structures is in most cases absolutelywrong. Coupled with optical and radio observations, these X-ray datashow evidence for violent mechanisms. Results based on XMM-Newton gastemperature maps for four clusters will be presented here.


Type
Research Article
Information
European Astronomical Society Publications Series , Volume 20: Mass Profiles and Shapes of Cosmological Structures , 2006 , pp. 183 - 186
Copyright
© EAS, EDP Sciences, 2006

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)