What May We Learn from Multi-Wavelength Observations of Active Galactic Nuclei

Courvoisier, Thierry J.-L.

doi:10.1007/10719740_14

Thierry J.-L. Courvoisier^1,2

Part of the book series: ESO ASTROPHYSICS SYMPOSIA ((ESO))

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Abstract.

We discuss how several of the questions that remain unclear on the physics of Active Galactic Nuclei may find elements of answers when using in the coming years the extraordinary set of instruments that will be flying simultaneously to observe in all bands of the electromagnetic spectrum. The choice of questions mentioned here is personal and not exhaustive.

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INTEGRAL Science Data Centre, 16 ch. d’Ecogia, CH-1290, VERSOIX, Switzerland
Thierry J.-L. Courvoisier
Observatoire de Genève, CH-1290, SAUVERNY, Switzerland
Thierry J.-L. Courvoisier

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Thierry J.-L. Courvoisier
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Giancarlo Setti Jean-Pierre Swings

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Courvoisier, T.JL. What May We Learn from Multi-Wavelength Observations of Active Galactic Nuclei. In: Setti, G., Swings, JP. (eds) Quasars, AGNs and Related Research Across 2000. ESO ASTROPHYSICS SYMPOSIA. Springer, Berlin, Heidelberg. https://doi.org/10.1007/10719740_14

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DOI: https://doi.org/10.1007/10719740_14
Published: 22 September 2003
Publisher Name: Springer, Berlin, Heidelberg
Print ISBN: 978-3-540-42191-7
Online ISBN: 978-3-540-45326-0
eBook Packages: Springer Book Archive

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