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Monthly Notices of the Royal Astronomical Society 391 (2008) 949-958
Measuring parameters of active galactic nuclei central engines with very high energy γ-ray flares
A. Neronov, D.V. Semikoz1, 2, S. Sibiryakov2

We discuss a "compact source" model of very high energy (VHE) emission from blazars in which the variability time is determined by the blazar central engine. In this model electron or proton acceleration close to the supermassive black hole is followed by the development of electromagnetic cascade in a radiatively inefficient accretion flow. Assuming such a model for the TeV blazar PKS 2155-304, we show that the variability properties of the TeV gamma-ray signal observed during a bright flare from this source, such as the minimal variability time scale and the recurrence period of the sub-flares, constrain the mass and the angular momentum of the supermassive black hole.
1 :  APC - UMR 7164 - AstroParticule et Cosmologie
2 :  Institute for Nuclear Research of the Russian Academy of Sciences
Physique/Astrophysique/Cosmologie et astrophysique extra-galactique

Planète et Univers/Astrophysique/Cosmologie et astrophysique extra-galactique
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