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Fig. 10

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Left panel: peculiar velocities of the main galaxies in groups with at least 12 member galaxies in superclusters of filament and spider morphology (red and blue lines), and in the field (grey line). Right panel: peculiar velocities of the main galaxies in groups with at least 12 member galaxies in superclusters of filament and spider morphology (red and blue dots) vs. environmental density in superclusters at smoothing length 8 h-1 Mpc.

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