Seyfert Galaxies

Seyfert galaxies would represent a transitional stage in the evolution of the universe. Seyfert galaxies would be younger than quasars, appearing in time after a full fledged quasar and yet, earlier than the formation of galaxies. Gradually, between the ancient quasars and our modern day galaxies, the Seyfert galaxies take on an intermediate role.

In our part of the universe, the formation of most galaxies was long ago completed. These far away Seyfert galaxies would showcase events and times after the pioneering quasars, but previous to the completed establishment of the structure of galaxies in our part of the universe.

By the C-R theory, a quasar evolves into, and becomes a Seyfert galaxy, then later, a fully established galaxy. The Seyfert galaxy essentially is to cosmological structure what the teens are to humans.

The C-R theory predicts that some of the Seyfert galaxies we are seeing now may still be in existence, due to the gravitationally slowed nature of the edges of the universe. The relatively "baby" quasars which we can see may now be aging, and evolving to enter their adolescent (cosmologically speaking) stages.

The transitional forms, from the quasars at edge of the universe, to our "fully formed?" Milky Way galaxy are open for viewing by any interested observer. Just as one can tell about the history of a family by viewing their photographic albums, one who is interested in the history of our universe need only look at the Milky Way's younger sibling galaxies, Seyfert galaxies, and quasars to see the progression of "nebular evolution".