  We have collected emission line ([Oiii] 5007 and Halpha+[Nii]) and radio
continuum images for a volume limited (cz <= 3600 km/s) sample of southern
Seyfert galaxies. The optical data were obtained at ESO using the 2.2 m, NTT
and 3.6 m telescopes, and have a typical resolution of 1" and noise level of
~1e-16 ergs cm-2 s-1 arcsec-2. The radio continuum observations were obtained
with the VLA (6 cm) and ATCA (3 cm) and have a resolution of ~1" matching that
of the optical images. All, but one of the observed sources were detected above
the noise limit of ~0.15 mJy.
  In the radio, 30% of the sources show linear structure, 25% are only slightly
resolved or diffused, and 45% remain unresolved at the ~1" resolution. As in
previous work, a correlation is found between the size of the radio structure
and the radio power. The radio sources in Seyfert 2 galaxies have, on average,
larger linear size than their type 1 counterparts, but there is no significant
difference in radio power between types 1 and 2. No significant difference is
found in the spectral indices of the two Seyfert types.
  Extended emission is common in Seyfert galaxies -- essentially all objects
observed show extended Halpha+[Nii] and nearly 50% show extended [Oiii]
emission. At least 40% (18 out of 50) of the galaxies show high excitation
extended emission line region (EELR) well outlined in the excitation map. The
EELR morphology vary from linear to conical to S-shaped and even X-shaped.
Almost exclusively all elongated EELR are in Seyfert 2 galaxies. The
orientation of the EELR appears to be random relative to either the major (or
minor) axis or relative to the non-axisymmetric structures, such as bars or
ovals, when present, and there is a hint of relation to the morphological type.
