  If the winds of an asymptotic-giant-branch stars are sufficiently strong are
slightly asymmetric, they can alter the star's trajectory through a globular
cluster; therefore, if these winds are asymmetric, one would expect young white
dwarfs to be less radially concentrated than either their progenitors or older
white dwarfs in globular clusters. This latter effect has recently been
observed. Additionally the young white dwarfs should have larger typical
velocities than their progenitors. After phase mixing this latter effect is
vastly diminished relative to the changes in the spatial distribution of young
white dwarfs with kicks, so it is more difficult to detect than the change in
the spatial distribution. The most powerful kinematic signature is the change
in the eccentricity of the orbits that is revealed through the distribution of
the position angles of proper motion.
