The high energy AGN continuum - Models without e+e- -pairs

Details The high energy AGN continuum - Models without e+e- -pairs The high energy AGN continuum - Models without e+e- -pairs

May 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992aipc..254..301k&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

6

Active Galactic Nuclei, Astronomical Models, Black Holes (Astronomy), Continuous Radiation, Electron-Positron Pairs, High Energy Interactions, Accretion Disks, Distribution Functions, Radio Emission, Steady State, Thermal Emission

Scientific paper

The general properties of the high energy AGN continuum are reviewed with particular emphasis on the connection between radio loud and radio quiet AGN in the broad context of the dynamics of accretion onto a black hole. Arguments are provided indicating the possibility that the emission from radio loud AGN originates at distances much larger than a few Schwarzschild radii from the black hole and hence the role of pairs in defining the observed spectrum is limited. A connection is made between the radio and high energy continuum of AGN.

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