  Analysis of ROSAT observations demonstrate that X-ray sources are associated
with bright Seyfert galaxies up to distances of about 40 arc min. These X-ray
sources are predominantly identified with blue stellar objects (BSO's) some of
which are already catalogued as quasars.
  The X-ray sources tend to pair and align across the nucleus of the active
Seyfert. Enough redshifts are now available to indicate similarities of the
redshifts in the quasar pairs and to enable computation of ejection velocities
of about 0.1c.
  BL Lac objects are a conspicuous kind of strong X-ray source which are
associated with Seyferts a high level of probability.The BL Lac's appear to be
a transition form between quasars and compact companion galaxies. Both quasars
and companion galaxies tend to align along the minor axis of the ejecting
galaxy and to extend to the same maximium separation of ~400 kpc.
  These observations require high redshift quasars to evolve into low redshift
companion galaxies. The initially high intrinsic redshift of the quasars must
then arise from the low particle masses in their recently created matter.
