Galaxy groups are more than an intermediate scale between clusters and halos hosting
individual galaxies, they are crucial laboratories capable of testing a range of astrophysics …

Despite major advances in climate science over the last 30 years, persistent uncertainties in
projections of future climate change remain. Climate projections are produced with …

In this paper, we investigate how massive central galaxies cease their star formation by
comparing theoretical predictions from cosmological simulations: EAGLE, Illustris, and …

We use the IllustrisTNG hydrodynamical simulations to show how the fractions of quenched
galaxies vary across different environments and cosmic time, and to quantify the role AGN …

We use the high-resolution TNG50 cosmological magnetohydrodynamical simulation to
explore the properties and origin of cold circumgalactic medium (CGM) gas around massive …

Jellyfish galaxies are prototypical examples of satellite galaxies undergoing strong ram
pressure stripping (RPS). We analyse the evolution of 512 unique, first-infalling jellyfish …

We analyse the physical properties of gas in the circumgalactic medium (CGM) of 132 Milky
Way (MW)-like galaxies at z= 0 from the cosmological magneto-hydrodynamical simulation …

We make an in-depth comparison of the IllustrisTNG cosmological simulations with
observed quenched fractions of central and satellite galaxies, for M stars= 109–12 M⊙ at …

Negative feedback from active galactic nuclei (AGN) is the leading mechanism for the
quenching of massive galaxies in the vast majority of modern galaxy evolution models …

We investigate how star formation quenching proceeds within central and satellite galaxies
using spatially resolved spectroscopy from the SDSS-IV MaNGA DR15. We adopt a …