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Fig. 6

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Spatial distribution of the cluster members, marked with squares and a size proportional to exp(δi) computed using the δi deviations obtained with the DS test. Red and blue correspond respectively to galaxies with lower and higher δi deviations from the mean, < δi >. The large black lines represent the directions of the velocity gradients in each cluster region. Crosses indicate the BCGs positions in each cluster.

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