Pair production in steady synchrotron self Compton models of active galactic nuclei.

Details Pair production in steady synchrotron self Compton models of active galactic nuclei. Pair production in steady synchrotron self Compton models of active galactic nuclei.

Jun 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997arbei..30....1l&link_type=abstract

Astrophysics Reports, Publications of the Beijing Astronomical Observatory, No. 30, p. 1 - 20

Astronomy and Astrophysics

Astrophysics

Active Galactic Nuclei: Particle Creation, Active Galactic Nuclei: X Rays, Active Galactic Nuclei: Radiation Mechanisms

Scientific paper

Steady synchrotron self Compton models are studied, assuming a constant injection of power law relativistic particles in a compact source embedded in a magnetic field. The produced γ-ray interacts with target photons of lower energies to produce relativistic electron positron pairs which radiatively cool before thermalizing and annihilating. The problem is treated numerically. During the model analysis, the author improves on earlier investigations and computes detailed emergent spectra for a wide range of parameters, and compares his results to the data from active galactic nuclei.

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