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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 3.

Theoretical S-curves at the λEdd–Σ plane, at the literature black hole mass of Mkn 590 and at R = 6, 20, 100 RSchw, color-coded by αB. The shaded band marks the empirical CL transition Eddington ratios from A. Jana et al. (2025), and the cross-hatched strip those from B. Palit et al. (2026).The empirical thresholds intersect the theoretical knees only for αB ≈ 0.5–0.55 at the inner radii. Black dashed lines correspond to S-curves predicted from standard accretion theory prescribed with α = 0.1.

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