Author:
BINGHAM R.,KELLETT B. J.,DE ANGELIS U.,TSYTOVICH V. N.,SHUKLA P. K.
Abstract
AbstractX-ray and extreme ultraviolet emission from galaxy clusters can be interpreted as thermal emission from a hot plasma gravitationally bound to the cluster and constituting a significant amount of the mass of the cluster. The origin of this plasma and its thermal energy content can be linked to the formation process through the theory of self-organization of these structures.
Publisher
Cambridge University Press (CUP)