Mergers are the mechanisms by which galaxy clusters are
assembled through the hierarchical growth of smaller clusters and
groups. Major cluster mergers are the most energetic events in the
Universe since the Big Bang. Many of the observed properties of
clusters depend on the physics of the merging process. These
include substructure, shock, intra cluster plasma temperature and
entropy structure, mixing of heavy elements within the intra
cluster medium, acceleration of high-energy particles, formation of
radio halos and the effects on the galaxy radio emission.
This book reviews our current understanding of cluster merging
from an observational and theoretical perspective, and is
appropriate for both graduate students and researchers in the
field.
General
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