Between z≈4.4 and 2.7, a simulated protocluster's cold circumgalactic gas is destroyed from the inside out by a merger and AGN feedback, while its Lyman-alpha halo shifts from filamentary to spherical.
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The birth of the intracluster medium: the evolution of multiphase gas and Lyman-$\alpha$ haloes in a simulated $z\sim3$ protocluster
Between z≈4.4 and 2.7, a simulated protocluster's cold circumgalactic gas is destroyed from the inside out by a merger and AGN feedback, while its Lyman-alpha halo shifts from filamentary to spherical.