CHEX-MATE: Exploring the kinematical properties of Planck galaxy clusters

Open Access

Fig. 12.

Radial velocity anisotropy profiles for the stacked clusters, where the stacking is in bins of $M_{500}^{SZ}$ $M_{500}^{\mathrm{SZ}}$ . The structure is exactly as in Fig. 11. In all plots, the vertical dashed lines indicate r₅₀₀ as obtained from the average $M_{500}^{SZ}$ $M_{500}^{\mathrm{SZ}}$ of the corresponding mass bin.

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