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Fig. 8

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Number of close neighbours per principal galaxy as a function of group richness . Dots and squares refer to red, passive and blue, star-forming principal galaxies, respectively. The solid line is the best error-weighted least-squares linear fit to the red principal galaxies data. The dashed line is the average number of close neighbours per blue galaxy if it is assumed independent of . The arrows mark the three ranges of richness probed.

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