Accretion disk-driven jet precession in active galactic nuclei

Details Accretion disk-driven jet precession in active galactic nuclei Accretion disk-driven jet precession in active galactic nuclei

Mar 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990a%26a...229..424l&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 229, no. 2, March 1990, p. 424-426.

Statistics

Computation

11

Accretion Disks, Active Galactic Nuclei, Black Holes (Astronomy), Extragalactic Radio Sources, Quasars, Radio Jets (Astronomy), Angular Momentum, Astronomical Models, Computational Astrophysics, Accretion Disks, Black Holes, Galaxies: Jets Of, Quasars: Jets Of

Scientific paper

The disk-driven precession model, proposed originally for SS433 by
Sarazin et al. (1980), is applied to extragalactic radio jets. By
presenting a statistical relationship between the precession period and
optical luminosity of the sources, it is shown that the observational
evidence is in favor of the model.

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