We present the first metal abundance profiles for a representative sample of massive
clusters. Our measurements extend to R 500 and are corrected for a systematic error …

Chemical enrichment of the Universe at all scales is related to stellar winds and explosive
supernovae phenomena. Metals produced by stars and later spread throughout the …

Hot atmospheres pervading galaxy clusters, groups, and early-type galaxies are rich in
metals, produced during epochs and diffused via processes that are still to be determined …

We present results from a 577 ks XMM–Newton observation of SPT-CL J0459–4947, the
most distant cluster detected in the South Pole Telescope 2500 square degree (SPT-SZ) …

The analysis of the elemental abundances in galaxy clusters offers valuable insights into the
formation and evolution of galaxies. In this study, we explore the chemical enrichment of the …

Aims. We study the chemical evolution of galaxy clusters by measuring the iron mass in the
ICM after dissecting the abundance profiles into different components. Methods. We used …

We present an X-ray spectral analysis using XMM-Newton/EPIC observations (∼ 100 ks) of
the merging galaxy cluster Abell 3365 (z= 0.093). Previous radio observations suggested …

Cuciti, V., Brunetti, G., van Weeren, R., et al. 2018, A&A, 609, A61 Cuciti, V., Cassano, R.,
Brunetti, G., et al. 2021a, A&A, 647, A51 Cuciti, V., Cassano, R., Brunetti, G., et al. 2021b …

In this Thesis I focus on the chemical enrichment of galaxy clusters by tracing the evolution
of iron in the intracluster medium (ICM) through high-angular resolution X-ray observations …

Clusters of galaxies are the largest gravitationally bound systems in the Universe. Their
immense gravitational potential holds 10's to 100's bright galaxies and also an intracluster …