Electron injection break and pair content of quasar jets

Details Electron injection break and pair content of quasar jets Electron injection break and pair content of quasar jets

Dec 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aipc..599..510b&link_type=abstract

X-RAY ASTRONOMY: Stellar Endpoints,AGN, and the Diffuse X-ray Background. Edited by Nicholas E. White, Giuseppe Malaguti, and G

Astronomy and Astrophysics

Astronomy

Quasars, Jets And Bursts, Galactic Winds And Fountains, X-Ray Sources, X-Ray Bursts

Scientific paper

We study the dependence of nonthermal radiation spectra in OVV quasars on the location of the low energy break in the electron/positron injection function. We show that the high energy spectra produced during 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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