Abell 1914
(Feldmeier etal 2004)
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- Groups begin the stripping process, and the cluster tides amplify this into the diffuse intracluster light.
- Simulations show evolution from ICL w/ substructure at relatively high surface brightness to more diffuse ICL over time.
- We see hints of this
evolution in observed galaxy clusters, with examples of strong ICL
production associated w/ merging clusters.
- The Virgo ICL shows complex substructure, and reveals the intricate connection between ICL and galaxies.
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The Virgo Cluster
(Mihos et al 2005)
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