this morning in #astroph
"The birth of the intracluster medium: the evolution of multiphase gas
and Lyman-Ξ± haloes in a simulated z βΌ 3 protocluster" by J. Bennet et al.
https://arxiv.org/pdf/2603.16991
a nice simulated view using Arepo of how the typical thermodynamical and chemical structure of the intracluster medium is first formed around z=3, through the interplay of accretions, galaxy and AGN activity.














