  We present three-dimensional hydrodynamic simulations of the interaction of a
slow wind from an asymptotic giant branch(AGB) star and a jet blown by an
orbiting companion. The jet or "Collimated Fast Wind" is assumed to originate
from an accretion disk which forms via Bondi accretion of the AGB wind or Roche
lobe overflow. We present two distinct regimes in the wind-jet interaction
determined by the ratio of the AGB wind to jet momentum flux. Our results show
that when the wind momentum flux overwhelms the flux in the jet a more
dis-ordered outflow outflow results with the jet assuming a corkscrew pattern
and multiple shock structures driven into the AGB wind. In the opposite regime
the jet dominates and will drive a highly collimated narrow waisted outflow. We
compare our results with scenarios described by Soker & Rappaport (2000) and
extrapolate the structures observed in PNe and Symbiotic stars.
