Very High Energy Active Galactic Nuclei Synchrotron self-Compton Modeling Tour

2); (2) Department of Physics; Astronomy Durham University); C. Boisson (1); H. Sol (1); J.-P. Lenain (1; M. J. Ward (2) ((1) LUTH Observatoire de Paris-Meudon; M. K. Daniel (2); P. M. Chadwick (2)

arxiv: 0904.1660 · v1 · submitted 2009-04-10 · 🌌 astro-ph.CO · astro-ph.HE

Very High Energy Active Galactic Nuclei Synchrotron self-Compton Modeling Tour

J.-P. Lenain (1 , 2) , M. K. Daniel (2) , C. Boisson (1) , P. M. Chadwick (2) , H. Sol (1) , M. J. Ward (2) ((1) LUTH Observatoire de Paris-Meudon , (2) Department of Physics

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Astronomy Durham University)

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classification 🌌 astro-ph.CO astro-ph.HE

keywords activeenergygalactichighmodelingnucleiself-comptonsynchrotron

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The current very high energy (VHE; E>100GeV) experiments have tremendously increased the number of detected extragalactic sources. We present a synchrotron self-Compton modeling tour of the active galactic nuclei currently established as VHE emitters so far, and investigate possible correlations among the intrinsic and derived parameters.

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Very High Energy Active Galactic Nuclei Synchrotron self-Compton Modeling Tour

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