Fig. 8
Left: distance to the sample of RR Lyr stars, between 5 and 10 kpc, in a cone view. We did not find any apparent cluster or group in the RRab due to streams, except for the variables in the Galactic center. The solid and dashed lines have the same meaning as in Fig. 7. Right: spatial distribution in Galactic coordinates of the 39 RR Lyr found in tile b201.
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