  We present radio observations for 29 southern Seyfert galaxies selected from
a volume limited sample with cz<3600 km s^-1, and declination delta<0degr.
Objects with declination -30degr<delta<0degr were observed with the Very Large
Array (VLA) at 6 cm (4.9 GHz) and objects with delta<-30degr were observed with
the Australia Telescope Compact Array (ATCA) at 3.5 cm (8.6 GHz). Both the VLA
and the ATCA observations have a resolution of ~1arcsec. These new observations
cover more than 50% of the southern sample with all but two of the 29 objects
detected above our limit of 0.15 mJy. Combining these data with data available
from the literature gives almost 85% coverage of the southern sample and
further expands the radio observations of a distance limited sample by 22%.
Collecting additional sources from the literature, consisting of known Seyferts
with cz < 4600 km s^-1, we find that 38% of the sources are unresolved at
arcsecond resolution, and 34% have linear radio structure. Our results expand
upon and are consistent with earlier studies. We confirm a correlation between
the size of the radio structure and the radio luminosity. A comparison between
Seyfert types 1 and 2 finds that type 2s tend to have a larger linear size.
There is no statistically significant difference in radio power between types 1
and 2, although all the most powerful objects appear to be Seyfert 2's. No
significant difference has been found in the spectral indices.
