  We present deep images of the kpc-scale radio continuum emission in 14
edge-on galaxies (ten Seyfert and four starburst galaxies). Observations were
taken with the VLA at 4.9~GHz (6~cm). The Seyfert galaxies were selected from a
distance-limited sample of 22 objects (defined in paper~I). The starburst
galaxies were selected to be well-matched to the Seyferts in radio power,
recessional velocity and inclination angle. All four starburst galaxies have a
very bright disk component and one (NGC~3044) has a radio halo that extends
several kpc out of the galaxy plane. Six of the ten Seyferts observed have
large-scale (radial extent $\gapprox$1 kpc) radio structures extending outward
from the nuclear region, indicating that large-scale outflows are quite common
in Seyferts. Large-scale radio sources in Seyferts are similar in radio power
and radial extent to radio halos in edge-on starburst galaxies, but their
morphologies do not resemble spherical halos observed in starburst galaxies.
The sources have diffuse morphologies, but, in general, they are oriented at
skewed angles with respect to the galaxy minor axes. This result is most easily
understood if the outflows are AGN-driven jets that are somehow diverted away
from the galaxy disk on scales $\gapprox$1 kpc. Starburst-driven winds,
however, cannot be ruled out. More observational work is needed to determine
whether massive star formation is present at high enough rates to drive
galactic winds out to kpc scales in Seyfert galaxies.

Astrophysics