Modelling blazar radiation spectra Electron injection break and pair content of quasar jets

Details Modelling blazar radiation spectra Electron injection break and pair content of quasar jets Modelling blazar radiation spectra Electron injection break and pair content of quasar jets

1999-10-22

arxiv.org/abs/astro-ph/9910416v1

Astronomy and Astrophysics

Astrophysics

4 pages, to appear in the proceedings of the Bologna Conference on "X-ray Astronomy 1999: Stellar Endpoints, AGNs and the Diff

Scientific paper

We study the dependence of nonthermal radiation spectra in OVV quasars on location of the low energy break in the electron/positron injection function. We show that the high energy spectra produced during the outbursts are presumably superposed from two components, one resulting from Comptonization of emission lines, which dominates at MeV-GeV energies, and the other resulting from Comptonization of infrared radiation, which dominates in the X-ray band.

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