Four decades ago, the firm detection of an Fe-K emission feature in the X-ray spectrum of
the Perseus cluster revealed the presence of iron in its hot intracluster medium (ICM). With …

Galaxy groups host the majority of matter and more than half of all the galaxies in the
Universe. Their hot (10 7 K), X-ray emitting intra-group medium (IGrM) reveals emission …

We introduce the Cluster-EAGLE (c-eagle) simulation project, a set of cosmological
hydrodynamical zoom simulations of the formation of 30 galaxy clusters in the mass range of …

We analyse the IllustrisTNG simulations to study the mass, volume fraction, and phase
distribution of gaseous baryons embedded in the knots, filaments, sheets, and voids of the …

The hot intra-cluster medium (ICM) permeating galaxy clusters and groups is not pristine, as
it has been continuously enriched by metals synthesised in Type Ia (SNIa) and core …

Accurate and precise measurement of the masses of galaxy clusters is key to deriving robust
constraints on cosmological parameters. However, increasing evidence from observations …

The distribution of metals in the intra-cluster medium (ICM) encodes important information
about the enrichment history and formation of galaxy clusters. Here, we explore the metal …

Aims. We studied the star formation rate (SFR) in cosmological hydrodynamical simulations
of galaxy (proto-) clusters in the redshift range 0< z< 4, comparing them to recent …

We analyse cosmological hydrodynamical simulations of galaxy clusters to study the X-ray
scaling relations between total masses and observable quantities such as X-ray luminosity …

Suzaku measurements of a homogeneous metal distribution of Z∼ 0.3 Solar in the outskirts
of the nearby Perseus cluster suggest that chemical elements were deposited and mixed …