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Extreme Variability Reveals How the Eddington Ratio Regulates Coronal Power in Active Galactic Nuclei

  • Authors: Arghajit Jana, Claudio Ricci, Franz E. Bauer, Kriti Kamal Gupta, Benny Trakhtenbrot, Alessia Tortosa, Ruancun Li, Luis C. Ho, Richard Mushotzky, Hsiang-Kuang Chang, Yaherlyn Diaz, Georgios Dimopoulos, Kristína Kallová, Michael J. Koss, Stéphane Paltani, Matthew J. Temple

Arghajit Jana et al 2026 The Astrophysical Journal Letters 1007 .

  • Provider: AAS Journals

Caption: Figure 5.

Raction of total emission from i) warm corona, ii) hot corona, and iii) accretion disk as a function of Eddington ratio is shown in top, middle, and bottom panel, respectively. The emission from the warm corona, hot corona, and accretion is estimated in 10−7–0.5, 0.001–10, and 0.1–500 keV, respectively.

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