Fig. 17.
Two point correlation function for stars in a local volume (d < 1 kpc). Both the RPM sample (black) and the 6D (blue) control sample are shown, in addition to a 5D version of the latter (grey). There is an excess of stars at velocity scales smaller than 100 km s−1, and at scales larger than 400 km s−1 in the 5D case. The correlation in the RPM sample is fully compatible with the correlation in the 5D version of the control sample.
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