GeV耀变体长期光变曲线中同步辐射与逆康普顿分量的相关性
高能天体物理现象
2009-09-01 v1
摘要
为了探索高能亮耀变体的GeV波段(即逆康普顿分量)与光学波段(即同步辐射分量)之间的相关性,将费米伽马射线空间望远镜(FGST)监测的一批耀变体的光变曲线与自动光学监测望远镜(ATOM)记录的相应光变曲线进行了比较。本文给出了比较结果。
引用
@article{arxiv.0908.4577,
title = {Correlation between the synchrotron and the inverse-Compton components, in the longterm light curve of GeV blazars},
author = {Bagmeet Behera and Marcus Hauser and Stefan J. Wagner},
journal= {arXiv preprint arXiv:0908.4577},
year = {2009}
}
备注
4 pages, 3 figures, contribution to the 31st ICRC, Lodz, Poland, July 2009