Fig. 13
Comparison of the simulations with SAM expectations. a) The SFR of galaxy G1a in cluster A, B, and C (runs S1, S3, and S4, respectively) and galaxy G1c is depicted with solid lines. The dashed lines correspond to the SFR of galaxy G1c with standard prescriptions for RPS (Gunn & Gott 1972) and SF (Cora 2006). In b), the same comparison is shown for the time evolution of the galaxy colours.
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