Please use this identifier to cite or link to this item: http://hdl.handle.net/2381/39832
Title: Exploring accretion disk physics and black hole growth with regular monitoring of ultrafast active galactic nucleus winds
Authors: Pounds, Ken
Lobban, Andrew
Nixon, Chris
First Published: 22-Mar-2017
Publisher: Wiley
Citation: Astronomische Nachrichten, 2017, 338 (2-3), pp. 249-255
Abstract: Fifteen years of XMM-Newton observations have established that ultrafast highly ionized winds (UFOs) are common in radio-quiet active galactic nucleus (AGN). A simple theory of Eddington-limited accretion correctly predicts the typical velocity (∼0.1c) and high ionization of such winds, with observed flow energy capable of ejecting star-forming gas. An extended XMM-Newton observation of the archetypal UFO PG 1211+143 recently found a more complex flow pattern, suggesting that intensive XMM-Newton observations offer exciting potential for probing the inner accretion disk structure and super-massive black hole (SMBH) growth.
DOI Link: 10.1002/asna.201713338
ISSN: 0004-6337
eISSN: 1521-3994
Links: http://onlinelibrary.wiley.com/doi/10.1002/asna.201713338/abstract;jsessionid=2AB3EA7A741ED861F0856D8ABC5091B2.f04t03
http://hdl.handle.net/2381/39832
Embargo on file until: 22-Mar-2018
Version: Post-print
Status: Peer-reviewed
Type: Journal Article
Rights: Copyright © 2017, Wiley. Deposited with reference to the publisher’s archiving policy available on the SHERPA/RoMEO website.
Description: The file associated with this record is embargoed until 12 months after the date of publication. The final published version may be available through the links above.
Appears in Collections:Published Articles, Dept. of Physics and Astronomy

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