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Matter Clustering in Astrid: Reduced Baryonic Suppression from Realistic Black Hole Dynamics

  • Authors: Yanhui Yang, 焱辉 杨, Simeon Bird, Yihao Zhou, 亦豪 周, Tiziana Di Matteo, Rupert Croft, Yueying Ni, Nianyi Chen

Yanhui Yang et al 2026 The Astrophysical Journal Letters 1007 .

  • Provider: AAS Journals

Caption: Figure 3.

Cumulative released kinetic feedback energy density distribution as a function of BH mass. The color and line styles are the same as in Figure 1. Panels from left to right show results at z = 0, 0.5, 1, and 1.5. Total released kinetic feedback energy [i.e., Ukf(∞, z)] is annotated for each SV simulation in the corresponding color.

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