Image Details

Choose export citation format:

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 1.

Integrated thermal timescale tth,int (red dashed) and front propagation timescale tfp (blue solid) as a function of black hole mass, computed for λEdd = 0.01, R = 20 RSchw, and αB = 0.5. The shaded band marks typical observed CLAGN transition durations. The annotation in the upper left indicates the qualitative dependence of tfp on the model parameters held fixed in this figure.

Other Images in This Article
Copyright and Terms & Conditions

Additional terms of reuse