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Pair Production in AGN

Published online by Cambridge University Press:  07 August 2017

C. Done
Affiliation:
Institute of Astronomy, Madingley Road, Cambridge CB3 0HA, U.K.
A. C. Fabian
Affiliation:
Institute of Astronomy, Madingley Road, Cambridge CB3 0HA, U.K.

Extract

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The X-ray luminosity and variability of many AGN are sufficiently extreme that any hard γ-rays produced in the source will collide with the X-rays and create electron-positron pairs, rather than escape. A small region where vast amounts of energy are produced, such as an AGN, is an ideal place to accelerate particles to relativistic energies and so produce γ-rays by Compton scattering. The observed X-ray spectra of AGN are hard and indicate that most of the luminosity is at the highest energies so that absorption of the γ-rays represents a large fraction of the energy flux, which can then be re-radiated at lower energies. Pairs can thus effectively reprocess much of the radiant power in an AGN.

Type
Part 3: X-rays and the Central Source
Copyright
Copyright © Kluwer 1989 

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