Waldek was interested in this subject during the 2002/2003 academic year. Any students
interested in this theme, please edit this page a translate this to a page FormacjiGalAGN w po polsku.
background:
FLRW model
unified AGN model
galaxy formation model
small density perturbations of about 10^{-5} at z=1100 grow with time
by gravitational collapse and form dark matter (baryonic + non-baryonic)
haloes, which merge and become successively larger