Hydrangea simulations show over 85% of S0 galaxies are cluster satellites formed primarily by environmental stripping of spirals rather than mergers.
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Characterizing the Formation and Evolution of S0-galaxies (CaFES-0): Their formation pathways around Galaxy Clusters
Hydrangea simulations show over 85% of S0 galaxies are cluster satellites formed primarily by environmental stripping of spirals rather than mergers.