The effect of the broad-line region with geometrical structures on gamma-ray absorption in blazars
arXiv:1308.4210 · doi:10.1093/pasj/pst008
Abstract
The broad-line region (BLR) is an important component of blazars, especially for the flat spectrum radio quasars (FSRQs). The soft photons arising from the BLR will substantially affect the transparency of the gamma-ray photons produced in the relativistic jet. In the paper, we study the effect of the geometrical structure of the BLR on the absorption of gamma-rays. We find that the gamma-ray optical depth strongly depends on the geometrical structure of the BLR. For a "flat" geometry of the BLR, the gamma-ray photons with specified energies could escape transparently even their emission region locates inside the cavity of the BLR.
16 pages, 7 figures, accepted by PASJ
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- The mystery of spectral breaks: Lyman continuum absorption by photon-photon pair production in the Fermi GeV spectra of bright blazars
- Properties of the narrow line Seyfert 1 galaxies revisited
- Modeling the spectral-energy-distribution of 3C 454.3 in a "flat" broad-line-region scenario
- Imprint of "Local Opacity" Effect in Gamma-Ray Spectrum of Blazar Jet
- Location of gamma-ray flaring region in quasar 4C +21.35
- Revisiting Correlations Between Broad-Line and Jet Emission Variations for AGNs: 3C 120 and 3C 273