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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 A1.

Scatterplot of BH mass (MBH) versus halo mass (M500c), colored by the cumulative released kinetic feedback energy Ekf. The first and second rows show the relation at z = 0 and z = 1, respectively. The four columns correspond to the four different SV simulations. Color circles represent BHs that have released kinetic feedback energy, while gray points represent BHs that have not released kinetic feedback energy.

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