We present spectra and high-resolution images taken with the Hubble Sp
ace Telescope (HST), the NTT, the VLA, and the MPIA/ESO 2.2 m telescop
e of the emission-line star He 3-1475, which we suggest is a postasymp
totic giant branch star. The star is presumed to be at the origin of a
15 '' long structure containing symmetrically opposing bright knots.
The knots have radial velocities of +/-500 km s(-1) from the center of
He 3-1475 to the ends of the jets. HST snapshots show that the core o
f He 3-1475 is unipolar with a star at the SE end and the nebula fanni
ng out toward the NW. VLA observations show the presence of OH masers,
which are positioned parallel to the optical jets. A model is propose
d that accounts for all of the observational data. This unusual object
may link the OH/IR stars having extreme outflow velocities with highl
y bipolar planetary nebulae. circumstellar