The distribution on the sky of clusters of galaxies shows significant
association with relatively nearby, large, active galaxies. The pattern is that
of clusters paired equidistant across a central galaxy with the apparent
magnitudes and redshifts of their constituent galaxies being closely matched.
The clusters and the galaxies in them tend to be strong X-ray and radio
emitters and their redshifts occur at preferred redshift values. The central,
low redshift galaxies often show evidence of ejection in the direction of these
higher redshift clusters and the clusters often show elongation along these
lines. In most of these respects the clusters resemble quasars which have been
increasingly shown for the last 34 years to be similarly associated with active
parent galaxies. It is argued here that, empirically, the quasars are ejected
from active galaxies. They evolve to lower redshift with time, fragmenting at
the end of their development into clusters of low luminosity galaxies. The
cluster galaxies can be at the same distance as their lower redshift parents
because they still retain a component of their earlier, quasar intrinsic
redshift.Comment: to be electronically publshed as XXXVI Recontres de Moriond, 200
