What does the nucleus look like?
Not to scale!

To achieve the necessary luminosity, ~ 1-10 Msun/yr must be accreted onto the black hole.
Under this model, Seyfert galaxies, radio galaxies, and quasars are similar objects -- accretion powered active nuclei. They may differ in total luminosity (quasars vs seyferts) or in radio power (seyferts vs quasars/radio galaxies) or in host galaxies (seyferts vs radio galaxies).
Question: how does this model "unify" Seyfert 1
and Seyfert 2 galaxies?
Hint: think viewing angle.
Is there direct observational support for this?

1. What do the host galaxies
of quasars look like?

These disturbed hosts suggest that quasars form when galaxies are experiencing interactions or gravitational perturbations.
2. When were quasars most
active?
We can look at the distribution in redshift of quasars. They occur much more frequently at high redshift, meaning they are very far away, so we are seeing them as they were long ago. We are actually looking at the early universe.
(courtesy Bill Keel, University of Alabama)
Quasars formed when the universe was young, probably coincident with the violence associated with galaxy formation. They quickly died out after that -- only a very few remain.Question: If quasars are associated with galaxy formation, what should we find in the centers of nearby galaxies?