Synchrotron-Self Compton Spectral Evolution of PKS 2155-304

2); 2) ((1) Physics Department & Astronomical Observatory; (2) INFN Perugia Section; Gino Tosti (1; Italy; Italy); Perugia; Stefano Ciprini (1; University of Perugia

arxiv: astro-ph/0303107 · v1 · submitted 2003-03-05 · 🌌 astro-ph

Synchrotron-Self Compton Spectral Evolution of PKS 2155-304

Stefano Ciprini (1 , 2) , Gino Tosti (1 , 2) ((1) Physics Department & Astronomical Observatory , University of Perugia , Italy , (2) INFN Perugia Section , Perugia

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keywords spectraldistributionavailablebeenbehaviorblazarbrightestcompton

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The high frequency peaked blazar PKS 2155-304 is one of the brightest and most intensively studied prototype of BL Lac objects. Gamma-rays from PKS 2155-304 have been detected from the MeV to TeV ranges. We computed a synchrotron self-Compton (SSC) model, based on the temporal behavior of the particles distribution, responsible for the high-energy emission. Using the available simultaneous multiwavelength data, we simulated the overall spectral energy distribution (SED) and the spectral variability of this source.

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Synchrotron-Self Compton Spectral Evolution of PKS 2155-304

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