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
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D O I：
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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.
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页码：269 / 272
页数：4
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