甚高能活动星系核的同步自康普顿模型巡礼
宇宙学与河外天体物理
2009-11-05 v1 高能天体物理现象
摘要
当前的甚高能(VHE; E>100GeV)实验极大地增加了已探测到的河外源的数量。我们对目前已被确认为VHE辐射体的活动星系核进行了同步自康普顿模型巡礼,并研究了内在参数与导出参数之间可能存在的相关性。
引用
@article{arxiv.0904.1660,
title = {Very High Energy Active Galactic Nuclei Synchrotron self-Compton Modeling Tour},
author = {J. -P. Lenain and M. K. Daniel and C. Boisson and P. M. Chadwick and H. Sol and M. J. Ward},
journal= {arXiv preprint arXiv:0904.1660},
year = {2009}
}
备注
4 pages, 5 figures. Contribution to the proceedings of the 2nd Heidelberg Workshop "High-Energy Gamma-rays and Neutrinos from Extra-Galactic Sources"