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Fig. 6.

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Number of star pairs per 0.5″ interval as a function of their angular separation. The dotted line gives the predicted distribution in the case of a spatially uniform distribution with the same average star density. Only stars within 600 pc of the Sun and with a Galactic latitude larger than 60° are considered here (1 233 947 stars). We measured about 29 000 pairs in excess of accidental pairs.

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