Astronomy and Astrophysics – Astrophysics
Scientific paper
Oct 1995
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995ap%26ss.232..307p&link_type=abstract
Astrophysics and Space Science, Volume 232, Issue 2, pp.307-313
Astronomy and Astrophysics
Astrophysics
Scientific paper
Research of several years has confirmed the general aspect that the most acceptable model in quasars' nuclei is a rotating Kerr black hole. Assuming the Kerr type potential given by the equation:
Mavrogiannis Manos
Petropoulos Basil
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