The innermost regions of Active Galactic Nuclei - from radio to X-rays

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dc.creatorRos, Eduardo
dc.creatorKadler, Matthias
dc.creatorKaufmann, Sarah
dc.creatorKovalev, Yuri Y.
dc.creatorTueller, Jack
dc.creatorWeaver, Kimberly A.
dc.date2006-11-16
dc.date.accessioned2026-07-07T07:30:51Z
dc.date.available2026-07-07T07:30:51Z
dc.descriptionActive Galactic Nuclei (AGN) 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 NGC1052. Beyond these studies, we address the latest technical developments and its impact in the AGN field: the Square Kilometre Array (SKA), a new radio interferometer planned for the next decade, and the oncoming X-ray and gamma-ray missions.
dc.descriptionTo appear in "Highlights of Spanish Astrophysics IV", Springer Verlag, ed. by F. Figueras, J.M. Girart, M. Hernanz, & C. Jordi; 12 pages, 1 figure with 5 panels, needs svmult.cls
dc.identifierhttps://arxiv.org/abs/astro-ph/0611530
dc.identifierhttp://arxiv.org/abs/astro-ph/0611530
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/118545
dc.subjectAstrophysics
dc.titleThe innermost regions of Active Galactic Nuclei - from radio to X-rays
dc.typetext

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