The innermost regions of active galactic nuclei - from radio to X-rays

被引：0

作者：

Ros, E. ^{[1
]}

Kadler, M. ^{[2
]}

Kaufmann, S. ^{[3
]}

Kovalev, Y. Y. ^{[1
,4
]}

Tueller, J. ^{[2
]}

Weaver, K. A. ^{[2
]}

机构：

[1] Max Planck Inst Radioastron, Hugel 69, D-53121 Bonn, Germany

[2] NASA, Goddard Space Flight Ctr, Astrophys Sci Div, Greenbelt, MD 20771 USA

[3] Univ Bonn, Argelander Inst Astron, D-53121 Bonn, Germany

[4] Ctr Astro Space, P N Lebedev Phys Inst, Moscow 117997, Russia

来源：

HIGHLIGHTS OF SPANISH ASTROPHYSICS IV | 2007年

基金：

俄罗斯基础研究基金会;

关键词：

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Active galactic nuclei can be probed by at different regions of the electromagnetic spectrum: e.g. radio observations reveal the nature of their relativistic jets and their magnetic fields, and complementarily, x-ray observations give insight into the changes in the accretion disk flows. Here we present an overview over the AGN research and results from an ongoing multi-band campaign on the active galaxy NGC 1052. Beyond these studies, we address the latest technical developments and its impact in the AGN field: the Square Kilometre Array, a new radio interferometer planned for the next decade, and the oncoming x-ray and gamma ray missions.

引用

页码：165 / +

页数：3

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