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GATOS: Distinct Feedback Modes in AGN Central Regions Revealed by Spatially Resolved JWST Spectroscopy

  • Authors: Lulu Zhang, Chris Packham, Erin K. S. Hicks, Ismael García-Bernete, Almudena Alonso-Herrero, Ric I. Davies, Martin J. Ward, Daniel E. Delaney, Takuma Izumi, Dimitra Rigopoulou, Cristina Ramos Almeida, Omaira González-Martín, Rogemar A. Riffel, Claudio Ricci, Montserrat Villar-Martín, Francoise Combes, Miguel Pereira-Santaella, Sebastian F. Hoenig, Andrew J. Bunker, Peter G. Boorman, Enrica Bellocchi, Nancy A. Levenson, Santiago García-Burillo, Fergus R. Donnan, Anelise Audibert, Lindsay Fuller, Tanio Díaz-Santos, David J. Rosario

Lulu Zhang et al 2026 The Astrophysical Journal Letters 1007 .

  • Provider: AAS Journals

Caption: Figure 6.

Illustrative schematic showing the two regimes in our AGN targets affected by the two feedback modes associated with AGN irradiation and shock processing, respectively. Gray arrows in the lower right corner indicate the directions in theory of increasing overall PAH size and neutral fraction as the PAH band ratios change. Using star-forming regions as a baseline, AGN irradiation tends to drive the heating and ionization of PAH molecules, followed by the preferential photodestruction of smaller PAHs, leading to a population dominated by larger and more ionized PAHs. In contrast, shock processing appears to preferentially destroy ionized PAHs, resulting in a higher survival fraction of large and neutral PAHs.

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