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1887
3561356
How gas flows shape the stellar-halo mass relation in the EAGLE simulation
Author(s):
Mitchell, P.D.; Schaye, J
Published
2022
Publication type
Article / Letter to editor
Galaxies - evolution
Galaxies - formation
Galaxies - haloes
Galaxies - stellar content
Astrophysics - astrophysics of galaxies
Date issued
2022
Language
English
Is part of
Monthly Notices of the Royal Astronomical Society (2022), Vol. 511, no. 2, p. 2948-2967
hdl
1887/3561356
doi
10.1093/mnras/stab3339
URL
https://ui.adsabs.harvard.edu/abs/2022MNRAS.511.2948M
Persistent identifier url
https://hdl.handle.net/1887/3561356
Documents
01 - 2103.10966
version: Accepted Manuscript
Full text at Publisher's site
Open Access