  Spectroscopic observations have been carried out for eleven objects believed
to be planetary nebulae on the basis of their optical appearance. They were
discovered in an ongoing deep search for galaxies in the Southern Milky Way
(Kraan-Korteweg & Woudt 1994). The objects were observed with the 1.9m
telescope of the South African Astronomical Observatory during our program for
obtaining redshifts of obscured galaxies in the ``Zone of Avoidance''. Of the
eleven objects, three proved too faint for a definite classification, four were
galaxies with radial velocities between v=3920 km/s and v=14758 km/s, but four
were confirmed as planetary nebulae (PNE). Their relative line strengths and
radial velocities have been determined. The PNE are on average fairly large
(23''-30''). Two of them (PNG 298.3+06.7 and PNG 323.6-04.5) were previously
unknown; for these we show H_alpha and [OIII] images.
