A fundamental relation between mass, SFR and metallicity in local and high redshift galaxies
F. Mannucci, G. Cresci, R. Maiolino, A. Marconi, and A. Gnerucci

TL;DR
This paper reveals a fundamental relation connecting stellar mass, star formation rate, and metallicity in galaxies, showing it holds across different redshifts and explains the observed mass-metallicity evolution.
Contribution
It introduces the Fundamental Metallicity Relation (FMR) linking mass, SFR, and metallicity, and demonstrates its invariance up to z~2.5, providing a unified framework for galaxy evolution.
Findings
Local galaxies define a tight 3D surface in mass, SFR, metallicity space.
High redshift galaxies follow the same FMR up to z~2.5, with no evolution.
The FMR's scatter supports smooth gas accretion models.
Abstract
We show that the mass-metallicity relation observed in the local universe is due to a more general relation between stellar mass M*, gas-phase metallicity and SFR. Local galaxies define a tight surface in this 3D space, the Fundamental Metallicity Relation (FMR), with a small residual dispersion of ~0.05 dex in metallicity, i.e, ~12%. At low stellar mass, metallicity decreases sharply with increasing SFR, while at high stellar mass, metallicity does not depend on SFR. High redshift galaxies, up to z~2.5 are found to follow the same FMR defined by local SDSS galaxies, with no indication of evolution. The evolution of the mass-metallicity relation observed up to z=2.5 is due to the fact that galaxies with progressively higher SFRs, and therefore lower metallicities, are selected at increasing redshifts, sampling different parts of the same FMR. By introducing the new quantity…
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