Revisiting the fundamental metallicity relation with observation and simulation
Chengyu Ma, Kai Wang, Enci Wang, Yingjie Peng, Haochen Jiang, Haoran, Yu, Cheng Jia, Zeyu Chen, Haixin Li, Xu Kong

TL;DR
This study investigates the factors influencing galaxy metallicity, revealing that galaxy size correlates more strongly with metallicity than star formation rate, with implications from both observations and simulations across cosmic time.
Contribution
It demonstrates that galaxy size, rather than star formation rate, is a more significant predictor of gas-phase metallicity in galaxies, supported by observational and simulation data.
Findings
Galaxy size correlates more strongly with metallicity than stellar mass.
Star formation rate's influence on metallicity increases at higher redshifts.
Galaxy size affects metallicity through gravitational potential and gas inflow regulation.
Abstract
The gas-phase metallicity of galaxies is regulated by multiple astrophysical processes, which makes it a crucial diagnostic of galaxy formation and evolution. Beyond the fundamental mass-metallicity relation, a debate about the secondary galaxy property to predict the metallicity of galaxies arises. Motivated by this, we systematically examine the relationship between gas-phase metallicity and other galaxy properties, i.e. star formation rate (SFR) and galaxy size, in addition to stellar mass in both observation and simulation. We utilize the data from the MaNGA (Mapping Nearby Galaxies at Apache Point Observatory) survey and the TNG50 simulations. We find that the combination of with is in much stronger correlation to the metallicity than stellar mass alone, regardless of whether the SFR is included or not, in both observation and simulation.…
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