- Table 1:
The sample of OH PPN candidates.
- Table 2:
The strongest polarized OH features in PPN candidates.
- Table 3:
The p-flux-weighted average polarization angle of
the linearly polarized OH maser emission at 1612 MHz and/or 1667 MHz
(PA1612, PA1667) and the position angle of nebula long axis
taken from optical and/or infrared or radio images.