  We present results of our search for collimated ionized winds in bipolar
nebulae using the Very Large Array (VLA) and the Australia Telescope Compact
Array (ATCA). Our search is motivated by the discovery of an ionized jet in the
bipolar nebula M 2-9 (Lim & Kwok 2003) that may be responsible for sculpting
the nebula's mirror-symmetric structure. To determine if such jets are a common
feature of bipolar nebulae, we searched for optically-thick radio cores - a
characteristic signature of ionized jets - in 11 northern nebulae with the VLA
at 1.3 cm and 0.7 cm, and in 5 southern nebulae with the ATCA at 6 cm and 3.6
cm. Two northern objects, 19W32 and M 1-91, and two southern objects, He2-84
and and Mz 3, exhibit a compact radio core with a rising spectrum consistent
with an ionized jet. Th 2-B exhibits a steeply falling spectrum characteristic
of nonthermal radio emission. Here we present a preliminary analysis of these
five radio cores and discuss the implications of our results.
