arXiv (OAI Expanded)
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The Connection between Halo Assembly History and the Stellar Distribution I: The Central Stellar Mass - Richness Plane
Recent observations suggest intrinsic links between the stellar components of massive halos and their assembly histories. Using massive halos with $\log[M_{\rm halo}/M_\odot] \geq 13.0$ from the IllustrisTNG-300 simulation, we explore differences in secondary halo properties between samples selected
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