Fig. 9
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Diagram of UVW velocities for TOI-1135 (gold star). The members of the Castor moving group (200–400 Myr), the Hyades super-cluster (Hs; 600–800 Myr), the IC 2391 supercluster (35–55 Myr), the Local Association (LA; 10–300 Myr), and the Ursa Major group (UMa; ~400 Myr) from Montes et al. (2001) are included. The ellipses represent the 3σ values of the UVW for each group.
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