Galaxies living in rich environments are suffering different perturbations able to drastically
affect their evolution. Among these, ram pressure stripping, ie the pressure exerted by the …

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 …

Context. How galaxies form, assemble, and cease their star formation is a central question
within the modern landscape of galaxy evolution studies. These processes are indelibly …

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

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 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 …

We compare the star-forming main sequence (SFMS) of galaxies–both integrated and
resolved on 1 kpc scales–between the high-resolution TNG50 simulation of IllustrisTNG and …

The TNG50 cosmological simulation produces X-ray emitting bubbles, shells, and cavities in
the circumgalactic gas above and below the stellar discs of Milky Way-and Andromeda-like …

Ultra-diffuse galaxies (UDGs) are the lowest-surface-brightness galaxies known, with typical
stellar masses of dwarf galaxies but sizes similar to those of larger galaxies such as the …

ABSTRACT We introduce Project GIBLE (Gas Is Better resoLved around galaxiEs), a suite of
cosmological zoom-in simulations where gas in the circumgalactic medium (CGM) is …