In TNG50, the resolved star-forming main sequence has slope 0.30, much shallower than observed, while the resolved mass-metallicity relation matches data; both can be described by a leaky-box model that prefers low net outflows.
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Star Formation Rates, Metallicities, and Stellar Masses on kpc-scales in TNG50
In TNG50, the resolved star-forming main sequence has slope 0.30, much shallower than observed, while the resolved mass-metallicity relation matches data; both can be described by a leaky-box model that prefers low net outflows.