We report the discovery of a collimated bipolar outflow emerging from a vis
ible disk around the proto-planetary nebula IRAS 17106-3046. The radius of
the disk, estimated to be 2500 AU at a distance of 4 kpc, is too large for
it to be a Keplerian disk created by accretion. The radial intensity profil
e of the disk suggests that it is consistent with an expanding torus. In co
ntrast to the open-end, butterfly-like lobes commonly seen in bipolar plane
tary nebulae, the lobes of IRAS 17106-3046 have pointed ends, suggesting a
recently formed jet breaking out of the lobes. IRAS 17106-3046 therefore co
uld represent the earliest stage of the bipolar-shaping process during the
transition from an asymptotic giant branch star to a planetary nebula.