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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 A1.

Diagnostic diagram of [Ne V] 14.32/PAH 11.3 (i.e., rNe) vs. H2 S(1–5)/PAH 7.7 (i.e., rH2) for ﹩0\mathop{.}\limits^{^{\prime\prime} }2\times 0\mathop{.}\limits^{^{\prime\prime} }2﹩ spaxels in the central ∼4″ × 4″ regions of the five AGN targets. The data points highlighted with black circles pertain to spaxels in NGC 7314 and Circinus with PAH 11.3/7.7 < 0.2 and PAH 6.2/7.7 < 0.15, while the points highlighted with red plus signs pertain to those with PAH 11.3/7.7 > 0.4.

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