不宁的类星体活动：从 BeppoSAX 到 Chandra 和 XMM-Newton
天体物理学
2009-11-10 v1
摘要
我们简要回顾了过去十年在类星体群体 X 射线性质研究方面取得的一些进展，从 BeppoSAX 观测到的明亮本地天体，到近年来 Chandra 和 XMM-Newton 探测到的迅速增长的大量 z>4 类星体。
引用
@article{arxiv.astro-ph/0309299,
title = {Restless Quasar Activity: From BeppoSAX to Chandra and XMM-Newton},
author = {C. Vignali and A. Comastri and W. N. Brandt},
journal= {arXiv preprint arXiv:astro-ph/0309299},
year = {2009}
}
备注
4 pages, 4 figures. To appear in the Proceedings of the Symposium "The Restless High-Energy Universe", 5-8 May 2003, Amsterdam, The Netherlands, E.P.J. van den Heuvel, J.J.M. in 't Zand, and R.A.M.J. Wijers Eds