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The nature of the soft X-ray emission in obscured AGN

Stefano Bianchi·Matteo Guainazzi
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Abstract

The origin of the soft X-ray emission in obscured AGN is still largely unknown. However, important progresses have been made thanks to the high energy and spatial resolution of XMM-Newton and Chandra. We review here the latest results on this issue, focusing on the physical properties of the material responsible for the soft X-ray emission and its relation to the circumnuclear environment, putting them in the general context of our understanding of the AGN structure and its feedback to the host galaxy.

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Stefano Bianchi, Matteo Guainazzi. 2006-11-02. The nature of the soft X-ray emission in obscured AGN. https://doi.org/10.1063/1.2774948

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