Fig. 5
Peculiar velocities of main cluster galaxies and the number of separate components in the clusters. Large symbols mark clusters with a non-Gaussian velocity distribution of galaxies (pAD < 0.05 and pSW < 0.05). Empty circles denote clusters with normalised peculiar velocities of their main galaxies Vpec,r < 0.5, filled circles denote clusters with Vpec,r > 0.5.
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