Transport of dust grain particles in the accretion disk
  Entrainment of dust particles in the flow inside and outside of the
proto-planetary disk has implications for the disk evolution and composition of
planets. Using quasi-stationary solutions in our star-disk simulations as a
background, we add dust particles of different radii in post-processing of the
results, using our Python tool DUSTER. The distribution and motion of particles
in the disk is followed in the cases with and without the backflow in the disk.
We also compare the results with and without the radiation pressure included in
the computation.
