We present a new model for the evolution of gas phase metallicity gradients in galaxies from
first principles. We show that metallicity gradients depend on four ratios that collectively …

We present a modified version of the l-galaxies2020 semi-analytic model of galaxy
evolution, which includes significantly increased direct metal enrichment of the …

Using the eagle (Evolution and Assembly of GaLaxies and their Environments) suite of
simulations, we demonstrate that both cold gas stripping and starvation of gas inflow play an …

We present an overview of the Middle Ages Galaxy Properties with Integral Field
Spectroscopy (MAGPI) survey, a Large Program on the European Southern Observatory …

We use a sample of z= 0 galaxies visually classified as slow rotators (SRs) in the eagle
hydrodynamical simulations to explore the effect of galaxy mergers on their formation …

The inflow of cosmological gas on to haloes, while challenging to directly observe and
quantify, plays a fundamental role in the baryon cycle of galaxies. Using the eagle suite of …

We analyse the evolution of the oxygen abundance gradient of star-forming galaxies with
stellar mass in the eagle simulation over the redshift range z=[0, 2.5]. We find that the …

Bars play an important role in mixing material in the inner regions of galaxies and
stimulating radial migration. Previous observations have found evidence for the impact of a …

We explore the properties of central galaxies living in voids using the eagle cosmological
hydrodynamic simulations. Based on the minimum void-centric distance, we define four …

We investigate the environmental dependence of the gas-phase metallicity for galaxies at z=
0 to z≳ 2 and the underlying physical mechanisms driving this dependence using state-of …