Modelling the multifrequency emission of blazars

Details Modelling the multifrequency emission of blazars Modelling the multifrequency emission of blazars

Jun 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002sf2a.conf..327k&link_type=abstract

SF2A-2002: Semaine de l'Astrophysique Francaise, meeting held in Paris, France, June 24-29, 2002, Eds.: F. Combes and D. Barret,

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Scientific paper

Synchrotron and inverse-Compton emission from inhomogeneous jets is quite successful in explaining multifrequency emission of blazars from low energy radio range to TeV energies, once correction for contamination by the host galaxy has been applied. In this frame, we considere two scenarios for VHE flares. Comparison with light curves obtained in radio and other low frequency range allows some test of the models, as we show for Mrk 421.

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