Unified Models of AGN Accretion Disks and Blazars

Details Unified Models of AGN Accretion Disks and Blazars Unified Models of AGN Accretion Disks and Blazars

Jan 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996aspc..110..384k&link_type=abstract

Blazar continuum variability Astronomical Society of the Pacific Conference Series 110, Proceedings of an international workshop

Astronomy and Astrophysics

Astrophysics

Accretion Disks, Active Galactic Nuclei, Blazars, Black Holes (Astronomy), Masks, Gamma Rays, Astrophysics

Scientific paper

Accretion disks around supermassive black holes are expected to be the power sources in all AGNS, including blazars. To date, though, little direct evidence for such disks exists in AGN observations. In blazars, the intense relativistic beaming would mask any underlying disk component. Here we present relevant work that our group at GMU is carrying out on unified aspects of disk accretion onto supermassive black holes and the possible coupling of thick disks to beams in the inner regions.

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