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Electromagnetic Observables of Weakly Collisional Black Hole Accretion

  • Authors: Vedant Dhruv, Cora Prather, Mani Chandra, Abhishek V. Joshi, Charles F. Gammie

Vedant Dhruv et al 2025 The Astrophysical Journal Letters 993 .

  • Provider: AAS Journals

Caption: Figure 4.

The 3 hr modulation index for all models considered in this work. The marker color represents the magnetization state (MAD versus SANE), while the marker shape indicates the black hole spin. Points below the dashed line represent models where the EGRMHD simulation produces 230 GHz light curves with lower variability than their ideal counterparts.

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