Barren but not Empty: The Impact of Void Environments on Galaxy and Halo Populations

arXiv:2608.26256 · astro-ph.GA, astro-ph.CO · Submitted 2026-08-26 · Read on arXiv

astro-ph.GA, astro-ph.CO

Submitted: 2026-08-26

Updated: 2026-08-26

Terminology

• Core — 48× in this paper · explained in 2 episodes
• AGN — 3× in this paper · explained in 1 episode
• Trace — 3× in this paper · explained in 2 episodes
• AGN Feedback — 1× in this paper · explained in 1 episode
• Abundance — 1× in this paper · explained in 1 episode
• Calibration — 1× in this paper · explained in 7 episodes
• Homogeneity — 1× in this paper · explained in 2 episodes
• Verification — 1× in this paper · explained in 2 episodes

Sources

• Anisotropic thermal conduction in galaxy clusters with MHD in Gadget
• Encyclopedia Magneticum: Scaling Relations from Cosmic Dawn to Present Day
• Why Cosmic Voids Matter: Nonlinear Structure & Linear Dynamics
• A hierarchy of voids: Much ado about nothing

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