Dianoga SIDM: Galaxy cluster self-interacting dark matter simulations

Open Access

Fig. 7.

Comparison between stacked velocity dispersion profiles. The top panel presents the stacked velocity dispersion profiles for our FP simulations of galaxy clusters in units of virial velocity $\sqrt{G M_{vir} / R_{vir}}$ $\sqrt{GM_{\mathrm{vir}}/R_{\mathrm{vir}}}$ . Bottom panel: ratios with respect to the DMO counterparts. Lines are coloured as in Fig. 4.

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