A Multiband Approach to AGN: Radioscopy & Radio Astronomy

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dc.creatorKadler, M.
dc.creatorRos, E.
dc.creatorKerp, J.
dc.creatorRoy, A. L.
dc.creatorMarscher, A. P.
dc.creatorZensus, J. A.
dc.date2004-11-18
dc.date.accessioned2026-07-07T02:15:55Z
dc.date.available2026-07-07T02:15:55Z
dc.descriptionOnly in the radio-loud population of active galactic nuclei (AGN) does the production, collimation, and acceleration of powerful relativistic jets take place. We introduce here a concept of combined VLBI- and X-ray spectroscopic observations of sources with relativistic, broad iron lines. This approach has enormous potential to yield deep insights into the accretion/jet-production process in AGN. Better knowledge of the milliarcsecond-resolution radio structure of the nuclear radio cores in so-called ``radio-quiet'' broad-iron-line Seyfert galaxies is essential for future combined radio/X-ray studies of the different modes of radio-jet production in accreting black hole systems.
dc.description4 pages, 1 figure, needes mem.cls, Proceedings contribution to the workshop "Multiband approach to AGN" held in Bonn (September 30 - October 2, 2004)
dc.identifierhttps://arxiv.org/abs/astro-ph/0411534
dc.identifierhttp://arxiv.org/abs/astro-ph/0411534
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/8597
dc.subjectAstrophysics
dc.titleA Multiband Approach to AGN: Radioscopy & Radio Astronomy
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