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A Magnetically Supported Disk–Corona Model for Changing-look Active Galactic Nuclei Transitions

  • Authors: Marios Kouzis, Agata Różańska, Debora Lančová, Bożena Czerny, Dominik Gronkiewicz

Marios Kouzis et al 2026 The Astrophysical Journal Letters 1007 .

  • Provider: AAS Journals

Caption: Figure 2.

Parametric grid of S-curves in the λEdd–Σ plane. Rows correspond to R = 6, 20, 100 RSchw (top to bottom). Columns span the magnetic viscosity from αB = 0.59 (left) to αB = 0.02 (right). Within each panel, line colors and styles denote MBH ∈ {107, 108, 109} M⊙, as marked in the box above.

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