具有相对论性喷流的窄线赛弗特 1 星系的基本性质
高能天体物理现象
2013-10-22 v2
摘要
我们展示了利用 Swift 卫星对一批射电 loud 窄线赛弗特 1 星系 (RLNLS1s) 样本进行巡天观测的初步结果。来自 Swift 的光学至 X 射线数据补充了来自 Fermi/LAT 的伽马射线观测以及文献中可用的射电测量数据。与一批明亮的 Fermi 耀变体样本的比较表明，RLNLS1s 似乎是该分布的低功率尾部。
引用
@article{arxiv.1301.0756,
title = {Basic properties of Narrow-Line Seyfert 1 Galaxies with Relativistic Jets},
author = {L. Foschini and E. Angelakis and G. Bonnoli and V. Braito and A. Caccianiga and L. Fuhrmann and L. Gallo and G. Ghirlanda and G. Ghisellini and D. Grupe and T. Hamilton and S. Kaufmann and S. Komossa and Y. Y. Kovalev and A. Lahteenmaki and M. L. Lister and K. Mannheim and L. Maraschi and S. Mathur and B. M. Peterson and P. Romano and P. Severgnini and G. Tagliaferri and J. Tammi and F. Tavecchio and O. Tibolla and M. Tornikoski and S. Vercellone},
journal= {arXiv preprint arXiv:1301.0756},
year = {2013}
}
备注
2 pages, 1 figure. Proceedings "X-ray Astronomy: the next 50 years" (Milano, 1-5 October 2012). To be published on Mem. SAIt. Errata-Corrige: found an error in the normalization of gamma-ray data. The old displayed values were luminosity densities (Lnu) instead of nuLnu. Now, the figures display the corrected values. Nothing changes in the concepts