The kinematical and space structures of IC 2391 open cluster and moving
  group with Gaia-DR2
  The kinematical parameters, spatial shape and structure of the open cluster
IC 2391 and the associated stellar stream are studied here using Gaia-DR2
(GDR2) astrometry data. The apex positions are determined for the open cluster
IC 2391 (data taken from Cantat-Gaudin et al.) and for the kinematical streams
stars mentioned in Montes et al. using both convergent point and AD-diagram
methods. The values of apex coordinates identified. The results are in good
agreement with the previously calculated values. The positions of the stars in
the disk and the spatial dispersion velocities are determined. The paths of
cluster and associated stream are traced in the disk by orbit calculation back
in time to their places of formation. A possible genetic relationship between
the cluster and the stream has been detected. The approximation of the spatial
and kinematical shape of the stream and the cluster is made. According to this
study, even though currently the cluster and the stream seem to have spatial
difference in their locations but they appear to have formed in the same region
of the Galactic disk.
