Fig. 16
The maroon solid and red dashed curves represent the velocity anisotropy profiles β(r) of the high- and low-M⋆ subsamples of passive cluster galaxies (above and below 1010.0M⊙). The shaded regions represents the corresponding 68% confidence levels. The vertical lines indicate the positions of r-2 (dashed) and r200 (dash-dotted).
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