The Blazar 3C 66A in 2003-2004: hadronic versus leptonic model fits

Details The Blazar 3C 66A in 2003-2004: hadronic versus leptonic model fits The Blazar 3C 66A in 2003-2004: hadronic versus leptonic model fits

Dec 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aipc.1085..502r&link_type=abstract

HIGH ENERGY GAMMA-RAY ASTRONOMY: Proceedings of the 4th International Meeting on High Energy Gamma-Ray Astronomy. AIP Conferenc

Astronomy and Astrophysics

Astronomy

5

Active And Peculiar Galaxies And Related Systems, Decays Of Leptons, Quasars, Active Or Peculiar Galaxies, Objects, And Systems

Scientific paper

The low-frequency peaked BL Lac object 3C 66A was the subject of an extensive multi-wavelength campaign from July 2003 till April 2004, which included quasi-simultaneous observations at optical, X-rays and very high energy gamma-rays. Here we apply the hadronic Synchrotron-Proton Blazar (SPB) model to the observed spectral energy distribution time-averaged over a flaring state, and compare the resulting model fits to those obtained from the application of the leptonic Synchrotron-Self-Compton (SSC) model. The results are used to identify diagnostic key predictions of the two blazar models for future multi-wavelength observations.

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