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Discovery of a dual AGN at z similar or equal to 3.3 with 20 kpc separation

  • A prediction of the current paradigm of the hierarchical assembly of galaxies is the presence of supermassive dual black holes at separations of a few kpc or less. In this context, we report the detection of a narrow-line emitter within the extended Ly alpha nebula (similar to 120 kpc diameter) of the luminous radio-quiet quasi-stellar object (QSO) LBQS 0302 0019 at z = 3 : 286. We identify several high-ionization narrow emission lines (He II, C IV, C III) associated with this point-like source, which we have named "Jil", which is only similar to 20 kpc (2 : 0 0 9) away from the QSO in projection. Emission-line diagnostics confirm that the source is likely powered by photoionization of an obscured active galactic nucleus (AGN) three orders of magnitude fainter than the QSO. The system represents the tightest unobscured/obscured dual AGN currently known at z > 3, highlighting the power of MUSE to detect these elusive systems.

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Author details:Bernd HusemannORCiD, Gabor WorseckORCiD, Fabrizio Arrigoni BattaiaORCiD, T. Shanks
DOI:https://doi.org/10.1051/0004-6361/201732457
ISSN:1432-0746
Title of parent work (English):Astronomy and astrophysics : an international weekly journal
Publisher:EDP Sciences
Place of publishing:Les Ulis
Publication type:Article
Language:English
Date of first publication:2018/01/13
Publication year:2018
Release date:2022/01/19
Tag:Techniques: imaging spectroscopy; Ultraviolet: ISM; galaxies: high-redshift; quasars: individual: LBQS 0302-0019
Volume:610
Number of pages:5
Funding institution:European Southern Observatory, Paranal, Chile [094.A-0767(A)]
Organizational units:Mathematisch-Naturwissenschaftliche Fakultät / Institut für Physik und Astronomie
DDC classification:5 Naturwissenschaften und Mathematik / 52 Astronomie / 520 Astronomie und zugeordnete Wissenschaften
Peer review:Referiert
Publishing method:Open Access / Bronze Open-Access
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