We present spectra and high-resolution images taken with the Hubble Space Telescope (HST), the NTT, the VLA, and the MPIA/ESO 2.2 m telescope of the emission-line star He 3-1475, which we suggest is a post-asymptotic 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 of He 3-1475 is unipolar with a star at the SE end and the nebula fanning out toward the NW. VLA observations show the presence of OH masers, which are positioned parallel to the optical jets. A model is proposed that accounts for all of the observational data. This unusual object may link the OH/IR stars having extreme outflow velocities with highly bipolar planetary nebulae.
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