Astronomy and Astrophysics – Astronomy
Scientific paper
May 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992aipc..254..105s&link_type=abstract
In: Testing the AGN paradigm; Proceedings of the 2nd Annual Topical Astrophysics Conference, Univ. of Maryland, College Park, Oc
Astronomy and Astrophysics
Astronomy
Active Galactic Nuclei, Astronomical Models, Big Bang Cosmology, Black Holes (Astronomy), Quasars, Origins, Particle Production, Plancks Constant, Relativistic Particles
Scientific paper
The paper examines the nature and origin of AGN using a Lemaitre-type model for the evolution of cosmic structures by the successive division processes of a compact 'primeval atom' at the Planck density in a series of regular stages during a period of slow inflation preceding the Big Bang. Typical superclusters have total masses of about 10 exp 15 solar masses, large galaxies of about 10 exp 12 solar masses, dwarf galaxies of about 10 exp 9 solar masses, globular clusters of about 10 exp 6 solar masses, stellar associations of about 1000 solar masses, and stars of about 1 solar mass. It is suggested that in the process of division by two of the original Lemaitre atoms there arise particularly long-lived clusters of pairs after every 10 steps on average with a Gaussian distribution around the mean of 10, portions of which survive for some time so as to serve as nuclei around which the various cosmological systems organize themselves.
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