As we have discussed, inner AGN
structure believed to feature a black
hole fed by an accretion disk.  Jets
may emerge along the spin axis,
and the disk illuminates BLR and
NLR clouds.  A dense molecular
torus exists on larger scales and
can obscure the central engine
from certain lines of sight.
“Unified Models” explain some of the different classes of AGN,
particularly type 1 and type 2 Seyferts, via orientation.
For specifics, see the Annual Reviews article by Antonucci, 1993, a
“bishop” in the “Church of Unification.”
Another nice website:
http://www.mssl.ucl.ac.uk/www_astro/agn/agn_unified.html