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Fig. B.1

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Cluster members’ relative position versus relative velocity with its slope at the angle of highest significance. The vertical black line shows the cluster’s median uncertainty in velocity. Panel (a): Trum- pler 14, (b): Trumpler 16, (c): CCCP-Cl 13, (d): Bochum 11, (e): IC 2581, (f): NGC 3324, (g): UBC 501
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