Galaxies and their dark-matter haloes have posed several challenges to the dark energy
plus cold dark matter (Λ CDM) cosmological model. These discrepancies between …

We discuss some of the key open questions regarding the formation and evolution of
globular clusters (GCs) during galaxy formation and assembly within a cosmological …

We select galaxies from the IllustrisTNG hydrodynamical simulations (at 0≤ z≤ 2) and
characterize the shapes and evolutions of their UVJ and star formation rate–stellar mass …

We use the Illustris simulation to study the relative contributions of in situ star formation and
stellar accretion to the build-up of galaxies over an unprecedentedly wide range of masses …

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

Abstract We introduce the MOdelling Star cluster population Assembly In Cosmological
Simulations within EAGLE (E-MOSAICS) project. E-MOSAICS incorporates models …

We use the IllustrisTNG simulations to study the demographics and properties of jellyfish
galaxies in the full cosmological context. By jellyfish galaxies, we mean satellites orbiting in …

Mergers and the spin of the dark matter halo are factors traditionally believed to determine
the morphology of galaxies within a Λ cold dark matter (ΛCDM) cosmology. We study this …

The Next Generation Virgo Cluster Survey (NGVS). XXX. Ultra-diffuse Galaxies and Their
Globular Cluster Systems - IOPscience This site uses cookies. By continuing to use this site you …

We present the first results from romulusc, the highest resolution cosmological
hydrodynamic simulation of a galaxy cluster run to date. romulusc, a zoom-in simulation of a …