XMM-NEWTON SCIENTIFIC HIGHLIGHTS: X-RAY SPECTROSCOPIC POPULATION STUDIES OF AGN

Authors

  • Matteo Guainazzi European Astronomy Center of the European Space Agency, Camino bajo del Castillo, s/n, Urbanización Villafranca del Castillo, Villanueva de la Cañada, E-28692 Madrid

DOI:

https://doi.org/10.14311/AP.2013.53.0626

Abstract

In this paper I review the contribution that the XMM-Newton ESA X-ray mission has given to our understanding of Active Galactic Nuclei, together with other operational, and complementary, X-ray facilities. I will focus on answering three basic questions: a) to which extent do AGN share the same engine?; b) to which extent are AGN “relativistic machines”?; c) to which extent do AGN affect their immediate environment?

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Published

2013-12-18

How to Cite

Guainazzi, M. (2013). XMM-NEWTON SCIENTIFIC HIGHLIGHTS: X-RAY SPECTROSCOPIC POPULATION STUDIES OF AGN. Acta Polytechnica, 53(A), 626–630. https://doi.org/10.14311/AP.2013.53.0626

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Articles