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Modeling the hard TeV spectra of blazars 1ES 0229+200 and 3C 66A with an internal absorption scenario

We study the applicability of the idea of internal absorption of gamma-rays produced through synchrotron radiation of ultrarelativistic protons in highly magnetized blobs to 1ES 0229+200 and 3C 66A, the two TeV blazars which show unusually hard intrinsic gamma-ray spectra after being corrected for the intergalactic absorption. We show that for certain combinations of reasonable model parameters, even with quite modest energy requirements, the scenario allows a self-consistent explanation of the non-thermal emission of these objects in the keV, GeV, and TeV energy bands.

preprint2011arXivOpen access
Olga ZacharopoulouDmitry KhangulyanFelix A. AharonianLuigi Costamante
astro-ph.HE
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Olga ZacharopoulouDmitry KhangulyanFelix A. AharonianLuigi Costamante

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