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- W2054253010 abstract "<i>Aims. <i/>Our goal is to understand the nature of blazars and the mechanisms for generating high-energy <i>γ<i/>-rays, through investigation of the blazar 3C 66A.<i>Methods. <i/>We model the high-energy spectrum of 3C 66A, which was observed recently with the Fermi-LAT and VERITAS telescopes. The spectrum has a hard change from the energy range of 0.2–100 GeV to 200–500 GeV in recent almost contemporaneous observations of two telescopes. <i>Results. <i/> The de-absorbed VERITAS spectrum depends strongly on redshift, which is highly uncertain. If <i>z<i/> = 0.444 is adopted, we are able to use the SSC model to produce the Fermi-LAT component and the EC model to the VERITAS component. However, if <i>z<i/> = 0.1, the intrinsic VERITAS spectrum will be softer, and there will be a smooth link between the Fermi-LAT and VERITAS spectra that can be explained using an SSC model." @default.
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- W2054253010 date "2010-02-01" @default.
- W2054253010 modified "2023-09-26" @default.
- W2054253010 title "Mechanism of very high-energy radiation in BL Lacertae object 3C 66A" @default.
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