Feedback effect on the observable properties of z > 6 AGN. Issue 2 (24th May 2022)
- Record Type:
- Journal Article
- Title:
- Feedback effect on the observable properties of z > 6 AGN. Issue 2 (24th May 2022)
- Main Title:
- Feedback effect on the observable properties of z > 6 AGN
- Authors:
- Vito, F
Di Mascia, F
Gallerani, S
Zana, T
Ferrara, A
Carniani, S
Gilli, R - Abstract:
- ABSTRACT: Active galactic nuclei (AGNs) feedback has a major impact on to the supermassive black hole (SMBH) growth, the properties of the host galaxies, and their cosmic evolution. We investigate the effects of different kinetic feedback prescriptions on the observable properties of AGN and their host galaxies at z > 6 in a suite of zoom-in cosmological simulations. We find that kinetic feedback decreases the column density of the interstellar medium (ISM) in the host galaxy by up to a factor of ≈10, especially when the SMBHs reach high accretion rates ($\approx 10{-}30\, \mathrm{M_\odot \, yr^{-1}}$ ). In particular, kinetic feedback is required to extend the ISM size to >1 kpc and match the observed sizes of the gas reservoirs in z > 6 AGN host galaxies. Moreover, it produces unobscured lines of sight along which the AGN can be detected in the rest-frame UV band with magnitudes consistent with observed values of z > 6 AGN. The assumed geometry of the outflow plays an important role in shaping the observed properties of high-redshift AGN. We find that a biconical geometry is favoured over a spherical one to reproduce the observed properties, but it overestimates the number of multiple AGN systems detectable in X-ray observations. This result suggests that simplistic BH seeding recipes widely employed in cosmological simulations produce too many X-ray detectable multiple AGN at z = 6−7, thus soliciting the adoption of more physically motivated seeding prescriptions.
- Is Part Of:
- Monthly notices of the Royal Astronomical Society. Volume 514:Issue 2(2022)
- Journal:
- Monthly notices of the Royal Astronomical Society
- Issue:
- Volume 514:Issue 2(2022)
- Issue Display:
- Volume 514, Issue 2 (2022)
- Year:
- 2022
- Volume:
- 514
- Issue:
- 2
- Issue Sort Value:
- 2022-0514-0002-0000
- Page Start:
- 1672
- Page End:
- 1688
- Publication Date:
- 2022-05-24
- Subjects:
- methods: numerical -- galaxies: active -- galaxies: high-redshift -- galaxies: nuclei -- early Universe
Astronomy -- Periodicals
Periodicals
520.5 - Journal URLs:
- http://mnras.oxfordjournals.org/ ↗
http://onlinelibrary.wiley.com/journal/10.1111/(ISSN)1365-2966 ↗
http://www.blackwell-synergy.com/issuelist.asp?journal=mnr ↗
http://www.blackwell-synergy.com/loi/mnr ↗
http://ukcatalogue.oup.com/ ↗ - DOI:
- 10.1093/mnras/stac1422 ↗
- Languages:
- English
- ISSNs:
- 0035-8711
- Deposit Type:
- Legaldeposit
- View Content:
- Available online (eLD content is only available in our Reading Rooms) ↗
- Physical Locations:
- British Library DSC - 5943.000000
British Library DSC - BLDSS-3PM
British Library HMNTS - ELD Digital store - Ingest File:
- 21821.xml