Fig. 10.
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Position (top left panel), magnitude-separation (top right panel), Gaia EDR3 PM-distribution (bottom left panel), and period-amplitude (bottom right panel) diagrams for the RR Lyrae stars located within 20′ from the centre of the cluster Patchick 125. The mean ridge lines for the Oosterhoff type I and II populations (left and right dotted lines, respectively) are from Clement & Shelton (1999). The two RR Lyrae members are shown as blue points.
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