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The effect of gas accretion on the radial gas metallicity profile of simulated galaxies

Florencia Collacchioni*, Claudia D. P. Lagos, Peter D. Mitchell, Joop Schaye, Emily Wisnioski, Sofia A. Cora, Camila A. Correa

*Corresponding author af dette arbejde

Publikation: Bidrag til tidsskriftTidsskriftartikelForskningpeer review

29 Citationer (Scopus)
44 Downloads (Pure)

Abstract

We study the effect of the gas accretion rate ((M) over dot)(accr)) on the radial gas metallicity profile (RMP) of galaxies using the eagle cosmological hydrodynamic simulations, focusing on central galaxies of stellar mass M-* greater than or similar to 10(9) M-circle dot at z

OriginalsprogEngelsk
TidsskriftMonthly Notices of the Royal Astronomical Society
Vol/bind495
Udgave nummer3
Sider (fra-til)2827-2843
Antal sider17
ISSN0035-8711
DOI
StatusUdgivet - 23 maj 2020

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