Abstract:
Seyfert galaxies are classified mainly into type 1 and type 2
depending on the presence and absence of broad permitted emission lines
in their optical spectra, respectively. Unification scheme hypothesizes that
the observed similarities and differences between the two Seyfert subtypes
can be understood as due to the differing orientations of anisotropically
distributed obscuring material having a torus-like geometry around
the AGN. We investigate the radio continuum emission properties of a
sample of Seyfert galaxies in the framework of the unification scheme
