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The Newcastle University research output collection, currently available on ePrints, will shortly be moving to a new open repository platform, Figshare. To prepare for the data migration we have paused adding new content to ePrints, and will resume once the new repository is launched. During this time you will continue to have access to ePrints (but no new content will appear). We will share updates here when available.

The resolved chemical abundance properties within the interstellar medium of star-forming galaxies at z≈ 1.5

Lookup NU author(s): Professor Chris 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): Gillman S, Puglisi A, Dudzevičiūtė U, Swinbank AM, Tiley AL, Harrison CM, Molina J, Sharples RM, Bower RG, Cirasuolo M, Ibar E, Obreschkow D

Publication type: Article

Publication status: Published

Journal: Monthly Notices of the Royal Astronomical Society

Year: 2022

Volume: 512

Issue: 3

Pages: 3480-3499

Print publication date: 01/05/2022

Online publication date: 07/03/2022

Acceptance date: 25/02/2022

Date deposited: 01/07/2022

ISSN (print): 0035-8711

ISSN (electronic): 1365-2966

Publisher: Oxford University Press

URL: https://doi.org/10.1093/mnras/stac580

DOI: 10.1093/mnras/stac580

ePrints DOI: 10.57711/djv1-d773


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Funding

Funder referenceFunder name
National Key R&D Program of China (2016YFA0400702)
National Science Foundation of China (11721303, 11991052)
ST/P000541/1
ST/T000244/1
STFC
ST/R504725/1

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