The fundamental plane of star formation in galaxies revealed by the EAGLE hydrodynamical simulations
Claudia del P. Lagos (ICRAR, CAASTRO), Tom Theuns (Durham), Joop, Schaye (Leiden), Michelle Furlong (Durham), Richard G. Bower (Durham),, Matthieu Schaller (Durham), Robert A. Crain (Liverpool), James W. Trayford, (Durham), Jorryt Matthee (Leiden)

TL;DR
This paper identifies a fundamental, nearly flat plane relating neutral gas fraction, stellar mass, and star formation rate in galaxies, consistent across redshifts and supported by both simulations and observations.
Contribution
It reveals a universal fundamental plane of star formation in galaxies, connecting key properties and supported by EAGLE simulations and observational data.
Findings
Galaxies form a nearly flat plane in $f_{gas, neutral}$-mass-SFR space.
The plane's position varies little with redshift, but galaxies move along it.
The plane's properties are consistent with observational data.
Abstract
We investigate correlations between different physical properties of star-forming galaxies in the "Evolution and Assembly of GaLaxies and their Environments" (EAGLE) cosmological hydrodynamical simulation suite over the redshift range . A principal component analysis reveals that neutral gas fraction (), stellar mass () and star formation rate (SFR) account for most of the variance seen in the population, with galaxies tracing a two-dimensional, nearly flat, surface in the three-dimensional space of with little scatter. The location of this plane varies little with redshift, whereas galaxies themselves move along the plane as their and SFR drop with redshift. The positions of galaxies along the plane are highly correlated with gas metallicity. The metallicity can…
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