On the structure of tidal tails
  We examine the longitudinal distribution of the stars escaping from a cluster along tidal tails. Using both theory and simulations, we show that, even in the case of a star cluster in a circular galactic orbit, when the tide is steady, the distribution exhibits maxima at a distance of many tidal radii from the cluster. 
Andreas H. W. K\"upper (1), Andrew Macleod (2) and Douglas C. Heggie   (2) ((1) Universit\"at Bonn, (2) University of Edinburgh)