Probing the AGN unification model at redshift z similar to 3 with MUSE observations of giant Ly alpha nebulae
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Date
2020-06
Publication Type
Journal Article
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yes
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Abstract
A prediction of the classic active galactic nucleus (AGN) unification model is the presence of ionization cones with different orientations depending on the AGN type. Confirmations of this model exist for present times, but it is less clear in the early Universe. Here, we use the morphology of giant Ly alpha nebulae around AGNs at redshift z similar to 3 to probe AGN emission and therefore the validity of the AGN unification model at this redshift. We compare the spatial morphology of 19 nebulae previously found around type I AGNs with a new sample of four Ly alpha nebulae detected around type II AGNs. Using two independent techniques, we find that nebulae around type II AGNs are more asymmetric than around type I, at least at radial distances r > 30 physical kpc (pkpc) from the ionizing source. We conclude that the type I and type II AGNs in our sample show evidence of different surrounding ionizing geometries. This suggests that the classical AGN unification model is also valid for highredshift sources. Finally, we discuss how the lack of asymmetry in the inner parts (r less than or similar to 30 pkpc) and the associated high values of the He II to Ly alpha ratios in these regions could indicate additional sources of (hard) ionizing radiation originating within or in proximity of the AGN host galaxies. This work demonstrates that the morphologies of giant Ly alpha nebulae can be used to understand and study the geometry of high-redshift AGNs on circumnuclear scales and it lays the foundation for future studies using much larger statistical samples.
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published
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Journal / series
Volume
495 (2)
Pages / Article No.
1874 - 1887
Publisher
Oxford University Press
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Date collected
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Subject
Galaxies: active; Galaxies: high-redshift; Intergalactic medium; Quasars: emission lines; Quasars: general
Organisational unit
03613 - Lilly, Simon (emeritus) / Lilly, Simon (emeritus)
09592 - Cantalupo, Sebastiano (ehemalig) / Cantalupo, Sebastiano (former)
Notes
It was possible to publish this article open access thanks to a Swiss National Licence with the publisher.
Funding
163824 - From Cosmic Web to Galaxies: Illuminating the Gaseous Link between the Dark and the Bright Universe (SNF)