2012
DOI: 10.1063/1.4772327
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Short term and multi-band variability of the active nucleus of IC310

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“…The short time-scales of variability impose severe constraints on the spatial extension of the emitting volume. The recent MAGIC observation of flares from the head-tail radio galaxy IC 310 with a variability time scale of approximately 4 minutes, is particularly puzzling as it requires an emission region more compact (by a factor of ≈ 5) than the Schwarzschild radius of the super massive black hole [34]. Another independent inference of a potentially even more compact size of the emission region in Blazars is possible using the effect of gravitational micro lensing [35].…”
Section: Gamma-rays From Active Galactic Nuclei and Gamma-ray Propaga...mentioning
confidence: 99%
“…The short time-scales of variability impose severe constraints on the spatial extension of the emitting volume. The recent MAGIC observation of flares from the head-tail radio galaxy IC 310 with a variability time scale of approximately 4 minutes, is particularly puzzling as it requires an emission region more compact (by a factor of ≈ 5) than the Schwarzschild radius of the super massive black hole [34]. Another independent inference of a potentially even more compact size of the emission region in Blazars is possible using the effect of gravitational micro lensing [35].…”
Section: Gamma-rays From Active Galactic Nuclei and Gamma-ray Propaga...mentioning
confidence: 99%