S. H. Beer and A. E. Vaughan
A search for planetary nebulae was carried out using candidates
selected by their infrared colours and 5 GHz radio emission.
One new planetary nebula was identified on the basis of its
small angular size, strong [OIII] emission and infrared colours.
Another object, known as the possible planetary nebula Wray 16-28,
is similarly identified as a planetary nebula.
An undiscovered AGN was also found, and is classed as a Seyfert 2
Galaxy on the basis of its strong OIII emission, linewidths of
500 km s-1, and 5 GHz radio flux.
Low-resolution optical spectra are presented and distance
estimates discussed.
Keywords: planetary nebulae: general -- galaxies: active -- galaxies: Seyfert