Time-Dependent Injection as a Model for Rapid Blazar Flares

被引：0
作者：
Zacharias, Michael [1 ]
机构：
[1] Heidelberg Univ, Landessternwarte, D-69117 Heidelberg, Germany
来源：
GALAXIES | 2016年 / 4卷 / 03期
关键词：
BL Lacertae objets; jets; gamma-rays; relativistic processes;
D O I：
10.3390/galaxies4030019
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Time-dependent injection can cause non-linear cooling effects, which lead to a faster energy loss of the electrons in jets. The most obvious result is the appearance of unique breaks in the SED, which would normally be attributed to a complicated electron distribution. Knowledge of the observation time and duration is important for the interpretation of the observed spectra, because of the non-trivial evolution of the spectral energy distributions (SED). Intrinsic gamma-gamma absorption processes in the emission region are only of minor importance.
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