Final answer:
According to the unified model of active galactic nuclei, a supermassive black hole is in the center surrounded by a rotating ring of dust, with a Type 1 Seyfert or Type 2 Seyfert being observed depending on the viewing angle.
Step-by-step explanation:
The unified model of active galactic nuclei states that a supermassive black hole is in the center surrounded by a rotating ring of dust. Depending on the viewing angle, we can observe either a Type 1 Seyfert or Type 2 Seyfert. The energy emitted from active galactic nuclei and quasars comes from material falling towards and forming a hot accretion disk around the supermassive black hole. Jets are seen in two directions, which are perpendicular to the accretion disk.