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Bridging Scales in Black Hole Accretion and Feedback: Subgrid Prescription from First Principles

  • Authors: Hyerin Cho, 혜린 조, Cora Prather, Ramesh Narayan, Kung-Yi Su, Angelo Ricarte, Priyamvada Natarajan, Antonio J. Porras-Valverde

Hyerin Cho et al 2026 The Astrophysical Journal Letters 1002 .

  • Provider: AAS Journals

Caption: Figure 3.

Distributions of ﹩\mathrm{ln}(\dot{M}/{\dot{M}}_{{\rm{B}}})﹩ (top row) and ﹩\mathrm{ln}(\eta )﹩ (bottom row). Each column is for a given BH spin a* and the blue and red curves are for the smallest and largest Bondi radii, RB ≈ 400 rg and ≈2 × 106 rg, respectively. Lognormal curves corresponding to each run are overplotted for comparison. The means of the lognormal variable X, calculated using Equation (D1) from log-space quantities ﹩{\mu }_{\mathrm{ln}X}﹩ and ﹩{\sigma }_{\mathrm{ln}X}﹩, are shown as vertical lines.

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