  We measure the angle between the neutron star (NS) natal kick direction and
the inferred direction of jets according to the morphology of 12 core collapse
supernova remnants (SNR), and find that the distribution is almost random, but
missing small angles.
  The 12 SNRs are those for which we could both identify morphological features
that we can attribute to jets and for which the direction of the NS natal kick
is given in the literature. Unlike some claims for spin-kick alignment, here we
rule out jet-kick alignment. We discuss the cumulative distribution function of
the jet-kick angles under the assumption that dense clumps that are ejected by
the explosion accelerate the NS by the gravitational attraction, and suggest
that the jet feedback explosion mechanism might in principle account for the
distribution of jet-kick angles.
