Fig. 1

U, V, and W recalculated velocities for the possible members of the Hyades Supercluster. Blue squares represent stars selected as members by the chemical tagging approach, red diamonds represent stars that have similar Fe abundances, but not for all the elements. Orange circles represent three Hyades cluster stars (BZ Cet, V683 Per, and ϵ Tau). Green triangles represent stars that do have similar Fe abundances (as well as similar values of other elements). The big black cross indicate the U, V, and W central location of the Hyades Supercluster (see Montes et al. 2001a). Dashed lines show the region where the majority of the young disk stars tend to be according to Eggen (1984, 1989).
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