Ultrafast outflows in ultraluminous X-ray sources
Ultrafast outflows in ultraluminous X-ray sources
Ultraluminous X-ray sources (ULXs) are bright extragalactic sources with X-ray luminosities above 1039 erg s−1 powered by accretion onto compact objects. According to the first studies performed with XMM-Newton, ULXs seemed to be excellent candidates to host intermediate-mass black holes (102 − 4M⊙). However, in the last years, the interpretation of super-Eddington accretion onto stellar-mass black holes or neutron stars for most ULXs has gained a strong consensus. One critical missing piece to confirm the super-Eddington scenario was the direct detection of the massive, radiatively driven winds expected as atomic emission/absorption lines in the ULX spectra. The first evidence for winds was found as residuals in the soft X-ray spectra of ULXs. Very recently, we have been able to resolve these residuals into rest-frame emission and blueshifted (∼ 0.2c) absorption lines arising from highly ionized gas in the deep, high-resolution XMM-Newton spectra of two ULXs. The compact object is therefore surrounded by powerful ultrafast winds as predicted by models of hyper-Eddington accretion. Here we discuss the relevance of these discoveries and the importance of further deep XMM-Newton observations of powerful winds in many other ULXs to estimate the energetics of the wind, the geometry of the system, and the masses of the central accretors.
234-240
Pinto, C.
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Fabian, A.
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Middleton, M.
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Walton, D.
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Pinto, C.
9d6e45cf-4900-42c4-8ca0-134c0af99af2
Fabian, A.
0c353376-f159-4129-b03e-d3993c0c5406
Middleton, M.
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Walton, D.
a1a36b18-a77b-48e8-8665-45bbef0c7bd1
Pinto, C., Fabian, A., Middleton, M. and Walton, D.
(2017)
Ultrafast outflows in ultraluminous X-ray sources.
Astronomische Nachrichten, 338 (2-3), .
(doi:10.1002/asna.201713336).
Abstract
Ultraluminous X-ray sources (ULXs) are bright extragalactic sources with X-ray luminosities above 1039 erg s−1 powered by accretion onto compact objects. According to the first studies performed with XMM-Newton, ULXs seemed to be excellent candidates to host intermediate-mass black holes (102 − 4M⊙). However, in the last years, the interpretation of super-Eddington accretion onto stellar-mass black holes or neutron stars for most ULXs has gained a strong consensus. One critical missing piece to confirm the super-Eddington scenario was the direct detection of the massive, radiatively driven winds expected as atomic emission/absorption lines in the ULX spectra. The first evidence for winds was found as residuals in the soft X-ray spectra of ULXs. Very recently, we have been able to resolve these residuals into rest-frame emission and blueshifted (∼ 0.2c) absorption lines arising from highly ionized gas in the deep, high-resolution XMM-Newton spectra of two ULXs. The compact object is therefore surrounded by powerful ultrafast winds as predicted by models of hyper-Eddington accretion. Here we discuss the relevance of these discoveries and the importance of further deep XMM-Newton observations of powerful winds in many other ULXs to estimate the energetics of the wind, the geometry of the system, and the masses of the central accretors.
Text
Ultrafast outflows in ultraluminous X-ray sources
- Accepted Manuscript
More information
Accepted/In Press date: 2 November 2016
e-pub ahead of print date: 29 March 2017
Additional Information:
Arxiv ref 1611.00623 Author confirms AM
Venue - Dates:
XXM-Newton: The Next Decade, , Madrid, Spain, 2016-05-09 - 2016-05-11
Organisations:
Astronomy Group
Identifiers
Local EPrints ID: 412017
URI: http://eprints.soton.ac.uk/id/eprint/412017
ISSN: 0004-6337
PURE UUID: 6a929446-d98f-4c98-a533-c686ec741d1f
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Date deposited: 05 Jul 2017 16:31
Last modified: 16 Mar 2024 05:30
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Author:
C. Pinto
Author:
A. Fabian
Author:
D. Walton
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