Cookies

We use cookies to ensure that we give you the best experience on our website. By continuing to browse this repository, you give consent for essential cookies to be used. You can read more about our Privacy and Cookie Policy.


Durham Research Online
You are in:

Obscured Active Galactic Nuclei

Hickox, R.C and Alexander, D.M. (2018) 'Obscured Active Galactic Nuclei.', Annual Review of Astronomy and Astrophysics, 56 . pp. 625-671.

Abstract

Active galactic nuclei (AGN) are powered by the accretion of material onto a supermassive black hole (SMBH) and are among the most luminous objects in the Universe. However, the huge radiative power of most AGN cannot be seen directly, as the accretion is hidden behind gas and dust that absorb many of the characteristic observational signatures. This obscuration presents an important challenge for uncovering the complete AGN population and understanding the cosmic evolution of SMBHs. In this review, we describe a broad range of multiwavelength techniques that are currently being employed to identify obscured AGN, and we assess the reliability and completeness of each technique. We follow with a discussion of the demographics of obscured AGN activity, explore the nature and physical scales of the obscuring material, and assess the implications of obscured AGN for observational cosmology. We conclude with an outline of the prospects for future progress from both observations and theoretical models, and we highlight some of the key outstanding questions.

Item Type:Article
Full text:Publisher-imposed embargo
(AM) Accepted Manuscript
File format - PDF
(5350Kb)
Status:Peer-reviewed
Publisher Web site:https://doi.org/10.1146/annurev-astro-081817-051803
Date accepted:01 June 2018
Date deposited:08 November 2021
Date of first online publication:20 July 2018
Date first made open access:No date available

Save or Share this output

Export:
Export
Look up in GoogleScholar