Simulation analysis finds ICL mostly from stripped intermediate-mass galaxies and BCGs from massive mergers, with overlapping but non-identical progenitors and distinct mass fractions, colors, and metallicities.
F., Faucher-Giguère, C.-A., et al
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Coevolution of Intracluster Light and Brightest Cluster Galaxies
Simulation analysis finds ICL mostly from stripped intermediate-mass galaxies and BCGs from massive mergers, with overlapping but non-identical progenitors and distinct mass fractions, colors, and metallicities.