Models of variability in blazar jets

被引：61

作者：

Mastichiadis, A ^{[1
]}

Kirk, JG

机构：

[1] Univ Athens, Dept Phys, GR-15784 Athens, Greece

[2] Max Planck Inst Kernphys, D-69029 Heidelberg, Germany

来源：

PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF AUSTRALIA | 2002年 / 19卷 / 01期

关键词：

acceleration of particles; radiation mechanisms : non-thermal; shock waves; galaxies : active;

D O I：

10.1071/AS01108

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

During the last decade multiwavelength observations of blazars have revealed many interesting patterns in their emission across the EM spectrum. In the present article we will review the time-dependent one-zone models and the models which advocate an acceleration and a radiation zone, and we will make some comparisons between them, especially in light of recent observations of the so-called TeV blazars.

引用

页码：138 / 142

页数：5

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