Fig. 10.
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Circular velocity profiles for FP simulations with a cluster centric distance < 0.15 Rvir. Each column shows a different matter component: total matter on the left, stellar component in the middle and the DM component on the right. Top panel: low mass regime [1, 2]×1010 h−1 M⊙, bottom panel: high mass regime [10, 40]×1010 h−1 M⊙. Line styles are as in Fig. 3.
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