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Within a 200 pc sphere around the Sun we search for the Hyades tidal tails inthe Gaia DR2 dataset. We use a modified convergent point method to search forstars with space velocities close to the space velocity of the Hyades cluster.We find a clear indication for the existence of the Hyades tidal tails, apreceding tail extending up to 170 pc from the centre of the Hyades with 292stars (36 contaminants), and a following tail up to 70 pc with 237 stars (32contaminants). A comparison with an N-body model of the cluster and its tailsshows remarkably good coincidence. Five white dwarfs are found in the tails.

The Hyades tidal tails revealed by Gaia DR2