Stability of turbulent synchro-Compton sources with respect to electron-positron pair production

Details Stability of turbulent synchro-Compton sources with respect to electron-positron pair production Stability of turbulent synchro-Compton sources with respect to electron-positron pair production

Oct 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987afz....27..371a&link_type=abstract

Astrofizika (ISSN 0571-7132), vol. 27, Oct. 1987, p. 371-381. In Russian.

Astronomy and Astrophysics

Astronomy

Active Galactic Nuclei, Compton Effect, Electron-Positron Pairs, Pair Production, Quasars, Radiation Sources, Positrons, Relativistic Electron Beams, Synchrotron Radiation

Scientific paper

It is confirmed that, in compact synchrotron sources with developed turbulence, electron acceleration can arise which leads to the formation of spectra of relativistic particles of a Maxwellian type with typical values of the Lorentz factor (gamma0) between 100 and 10,000. The relativistic particles, either directly or through secondary gamma rays, lead to the formation of electron-positron pairs . The results are of interest in connection with X-ray emission from active galactic nuclei and quasars.

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