Synchro-self-compton Radiation Mechanism Of Jets Of AGN With Ultra- And Moderate Relativistic Electrons

Details Synchro-self-compton Radiation Mechanism Of Jets Of AGN With Ultra- And Moderate Relativistic Electrons Synchro-self-compton Radiation Mechanism Of Jets Of AGN With Ultra- And Moderate Relativistic Electrons

Sep 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011xau5.confe..41n&link_type=abstract

"The Second Ferrara Workshop on "X-ray Astrophysics up to 511 keV", held in Ferrara (Italy), September 14 - 16, 2011, article #4

Astronomy and Astrophysics

Astrophysics

Scientific paper

New expressions are obtained for intensity of radiation of moderate relativistic electrons in a weak magnetic field. For ultrarelativistic electrons these expressions transform to well known formulae. With obtained earlier formulae for Compton scattering for arbitrary electron and photon energies the complete description of synchro-self-Compton radiation mechanism is given. Corresponding computer codes for calculation are written. The results can be used for interpretation of spectra of jets of active galactic nuclei and binary systems with black holes or neutron stars.

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