Galaxy clusters seen in X-rays: from the most relaxed to the most perturbed - CNRS - Centre national de la recherche scientifique Accéder directement au contenu
Communication Dans Un Congrès Année : 2005

Galaxy clusters seen in X-rays: from the most relaxed to the most perturbed

F. Durret
  • Fonction : Auteur
Lima Neto G. B.
  • Fonction : Auteur
J. Bagchi
  • Fonction : Auteur
W. Forman
  • Fonction : Auteur
E. Slezak
  • Fonction : Auteur
G. Soucail
  • Fonction : Auteur

Résumé

We present recent X-rays, optical and radio observations of the rich clusters of galaxies Abell 85, 496, 2667, and 3376. Detailed analysis of these clusters shows that none of them is strictly relaxed, all of them revealing to some degree signs of recent dynamical activity. We show how temperature maps and multi-wavelength observations are powerful tools to probe the history of galaxy clusters.
Fichier non déposé

Dates et versions

hal-00015560 , version 1 (09-12-2005)

Identifiants

  • HAL Id : hal-00015560 , version 1

Citer

F. Durret, Lima Neto G. B., C. Adami, J. Bagchi, G. Covone, et al.. Galaxy clusters seen in X-rays: from the most relaxed to the most perturbed. SF2A-2005: Semaine de l'Astrophysique Francaise, meeting held in Strasbourg, France, June 27 - July 1, 2005, 2005, France. pp.709. ⟨hal-00015560⟩
63 Consultations
0 Téléchargements

Partager

Gmail Facebook X LinkedIn More