GeV breaks in blazars as a result of gamma-ray absorption within the broad-line region

Abstract

Spectra of the brightest blazars detected by the Fermi Gamma-ray Space Telescope Large Area Telescope cannot be described by a simple power law model. A much better description is obtained with a broken power law, with the break energies of a few GeV. We show here that the sharpness and the position of the breaks can be well reproduced by absorption of gamma-rays via photon--photon pair production on HeII Lyman recombination continuum and lines. This implies that the blazar zone lies inside the region of the highest ionization of the broad-line region (BLR) within a light-year from a super-massive black hole. The observations of gamma-ray spectral breaks open a way of studying the BLR photon field in the extreme-UV/soft X-rays, which are otherwise hidden from our view.

4 pages, 3 figures, 2 tables; published in ApJ Letters

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• Bright AGN Source List from the First Three Months of the Fermi Large Area Telescope All-Sky Survey
• The redshift-dependence of gamma-ray absorption in the environments of strong-line AGN
• Intrinsic absorption in 3C 279 at GeV-TeV energies and consequences for estimates of the EBL

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