Variability studies and modelling of the blazar PKS 2155-304 in the light of a decade of multi-wavelength observations

被引:21
|
作者
Chevalier, J. [1 ]
Sanchez, D. A. [1 ]
Serpico, P. D. [2 ]
Lenain, J. -P. [3 ]
Maurin, G. [1 ]
机构
[1] Univ Savoie Mt Blanc, Univ Grenoble Alpes, CNRS, LAPP, F-74000 Annecy, France
[2] USMB, Univ Grenoble Alpes, CNRS, LAPTh, F-74940 Annecy, France
[3] Univ Paris Diderot, Sorbonne Univ, Sorbonne Paris Cite, CNRS,IN2P3,LPNHE, 4 Pl Jussieu, F-75252 Paris, France
关键词
galaxies: active; galaxies: individual: PKS2155-304; galaxies: jets; GAMMA-RAY FLARE; RADIATION; EMISSION; BINARIES; OBJECTS; FERMI; HESS;
D O I
10.1093/mnras/stz027
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The variability of the high-frequency peaked BL Lac object PKS 2155-304 is studied using almost 10 years of optical, X-ray and gamma-ray data. Publicly available data have been gathered and analysed with the aim to characterize the variability and to search for lognormality or periodic behaviour. The optical and X-ray range follow a lognormal process; a hint for a periodicity of about approximate to 700 d is found in optical and in the high energy (100 MeV < E < 300 GeV) range. A one-zone, time-dependent, synchrotron self-Compton model is successfully used to reproduce the evolution with energy of the variability and the tentatively reported periodicity.
引用
收藏
页码:749 / 759
页数:11
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