Synchrotron-self Compton spectral evolution of PKS 2155-304

被引：0

作者：

Ciprini, S ^{[1
]}

Tosti, G ^{[1
]}

机构：

[1] Univ Perugia, Dept Phys, I-06123 Perugia, Italy

来源：

HIGH ENERGY BLAZAR ASTRONOMY | 2003年 / 299卷

关键词：

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

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 multi-wavelength data, we simulated the overall spectral energy distribution (SED) and the spectral variability of this source.

引用

页码：269 / 272

页数：4

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