Axisymmetry in protoplanetary nebulae: using imaging polarimetry to investigate envelope structure

We use ground-based imaging polarimetry to detect and image the dusty circu mstellar envelopes of a sample of protoplanetary nebulae (PPNe) at near-inf rared wavelengths. This technique allows the scattered light from the faint envelope to be separated from the glare of the bright central star, and is particularly well suited to this class of object. We detect extended (up t o 9-arcsec diameter) circumstellar envelopes around 15 out of 16 sources wi th a range of morphologies including bipolars and shells. The distribution of scattered light in combination with its polarization (up to 40 per cent) provides unambiguous evidence for axisymmetry in 14 objects, showing this to be a common trait of PPNe. We suggest that the range of observed envelop e morphologies results from the development of an axisymmetric dust distrib ution during the superwind phase at the end of the AGE. We identify shells seen in polarized light with scattering from these superwind dust distribut ions, which allows us to provide constraints on the duration of the superwi nd phase. In one object (IRAS 19475 + 3119) the circumstellar envelope has a two-armed spiral structure, which we suggest results from the interaction of the mass-losing star with a binary companion.