Fig. 1.
Velocity distribution of the stars in the tangential velocity plane (V∥obs – V∥pred, V⊥obs). The zero-point is the predicted value from the space motion of the Hyades. The x-axis points in the direction of the convergent point. The units on the colour-bar are stars per (0.25 km s−1)2. The box indicates the selection window that might belong to the tails.
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