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Cosmological simulations predict that AGN preferentially live in gas-rich, star-forming galaxies despite effective feedback

Lookup NU author(s): Dr Christopher HarrisonORCiD

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This is the authors' accepted manuscript of an article that has been published in its final definitive form by Oxford University Press, 2022.

For re-use rights please refer to the publisher's terms and conditions.


Publication metadata

Author(s): Ward SR, Harrison CM, Costa T, Mainieri V

Publication type: Article

Publication status: Published

Journal: Monthly Notices of the Royal Astronomical Society

Year: 2022

Volume: 514

Issue: 2

Pages: 2936-2957

Print publication date: 01/08/2022

Online publication date: 03/05/2022

Acceptance date: 27/04/2022

Date deposited: 01/07/2022

ISSN (print): 0035-8711

ISSN (electronic): 0035-8711

Publisher: Oxford University Press

URL: https://doi.org/10.1093/mnras/stac1219

DOI: 10.1093/mnras/stac1219

ePrints DOI: 10.57711/d9hz-2e41


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Funding

Funder referenceFunder name
Deutsche Forschungsgemeinschaft (DFG, German Research Foundation) under Germany’s Excellence Strategy: EXC-2094-390783311
MR/V022830/1
UKRI

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