Kinematic structures found with Gaia DR1/TGAS and RAVE in the Solar
  neighbourhood
  With the much enlarged stellar sample of 55831 stars and much increased
precision in distances, proper motions, provided by Gaia DR1 TGAS we have shown
with the help of the wavelet analysis that the velocity distribution of stars
in the Solar neighbourhood contains more kinematic structures than previously
known. We detect 19 kinematic structures between scales 3-16 km/s at the 3sigma
confidence level. Among them we identified well-known groups (such as Hercules,
Sirius, Coma Berenices, Pleiades, and Wolf 630). We confirmed recently detected
groups (such as Antoja12 and Bobylev16). In addition we report here about a new
kinematic structure at (U,V)=(37, 8) km/s. Another three new groups are
tentatively detected, but require confirmation.
