Recent high-resolution observations of CO outflows often reveal well-c
ollimated emitting regions with radial velocities that increase away f
rom the outflow source (''accelerating'' outflows), surrounded by limb
-brightened low-velocity emission. There is growing evidence that mole
cular flows exhibiting this structure are driven by high-velocity, pos
sibly time-variable, narrow jets. In order to better understand the dy
namical interaction between such jets and the large-scale outflow, we
present a simple, analytic model in which the molecular outflow corres
ponds to environmental gas entrained in the wake of a bowshock created
by an internal jet working surface. This model results in flows with
velocity and density structures that appear to be similar to the obser
ved ''accelerating'' molecular flows. The model also gives global outf
low shapes that are comparable to the observed ones, and predicts a hi
gher collimation for less energetic flows (i.e. for lower luminosity s
ources), in agreement with reported trends.