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Fig. 2.


Dependence of the velocity segregation with the magnitude gap obtained using relative magnitudes. Top left panel: result obtained with all the galaxies within 1 R200, whereas in top right panel we use only galaxies within 0.5 R200. Lower panels: same results, but separating central galaxies (filled stars) from satellites. The remaining symbols and color code are the same as in Fig. 1.

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