Isolated central galaxies near massive halos are systematically more gas-poor than group centrals of the same black hole mass and star-formation offset, evidence for environment-driven gas removal.
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Even central galaxies feel their environment: cosmic siphoning of cool gas accretion
Isolated central galaxies near massive halos are systematically more gas-poor than group centrals of the same black hole mass and star-formation offset, evidence for environment-driven gas removal.