Fig. 4.
Gaia proper motion diagrams for previously known YSO members and the new disk-bearing YSOs presented in this paper. Upper panels: same new disk-bearing sources, bottom panels: new disk-bearing sources restricted to the respective spatial locations of Upper Sco and V1062 Sco. All panels show an ellipse corresponding to 5 σ of the mean proper motion of the respective confirmed members (the UCL ellipse is larger than the panel).
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