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Fig. 1.
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Revised galactocentric UVW velocities of GJ 1284 (blue), GJ 898 (orange), and GJ 897AB (green) from this work compared to other YMG members from Montes et al. (2001). The ellipses represent the 2σ values of UVW for each YMG. Similarly, we overplot βPMG and COL as defined by Gagné et al. (2018).
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