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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 5.

Same as Figure 4, but color-coded by the different strength indicators of (a) shock processing ([Fe II] 5.34/[Ar II] 6.99) and (b) AGN irradiation ([Ne V] 14.32/[Ne III] 15.56). The reddish and bluish crosses in panels (a) and (b) show, for the five AGN targets, the median PAH band ratios of the spaxels in bins of increasing log ([Fe II] 5.34/[Ar II] 6.99) of [−0.5, −0.25], [−0.25, 0], [0, 0.25], and [0.25, 0.5] and increasing log ([Ne V] 14.32/[Ne III] 15.56) of [−0.5, −0.3], [−0.3, −0.15], [−0.15, 0], and [0, 0.2] (from light to dark), respectively.

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