Synchrotron-Self Compton Spectral Evolution of PKS 2155-304

Details Synchrotron-Self Compton Spectral Evolution of PKS 2155-304 Synchrotron-Self Compton Spectral Evolution of PKS 2155-304

2003-03-05

arxiv.org/abs/astro-ph/0303107v1

ASP Conf.Ser. 299 (2003) 269

Astronomy and Astrophysics

Astrophysics

4 pages, 6 PS figures, 1 table. Poster at the International Workshop "High Energy Blazar Astronomy" celebrating the 50th anniv

Scientific paper

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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