Journal article icon

Journal article

The Galaxy Activity, Torus, and Outflow Survey (GATOS). XIII. Coupling Driven H 2 Excitation in Seyferts

Abstract:
We utilize James Webb Space Telescope/Mid Infrared Instrument (JWST/MIRI) Integral Field Unit observations from the Galaxy Activity, Torus and Outflow Survey to investigate the diverse range of ionized outflow rates of obscured active galactic nuclei (AGN) with similar bolometric luminosity and explore potential associations with AGN feedback. We explore spatial correlations between ionized emission potentially associated with fast shocks ([Fe II]5.34μm) and the excitation of H2. We further constrain our investigation to the inner 400 pc (the nuclear and circumnuclear regions r < 200 pc), and estimate the excitation temperature and column density of H2 assuming local thermodynamic equilibrium and using the S(1)–S(8) rotational H2 emission lines visible to JWST/MIRI spectroscopy. We report the molecular gas temperature of the deprojected 400 pc nuclear region to correlate with the ionized mass outflow rate. We also observe a stronger degree of spatial correlation between [Fe II]5.34μm emission and H2 gas temperature. We observe regions of enhanced [Fe II]5.34μm/[Ar II]6.99μm spatially coincident with the ionization cones of objects with higher ionized outflow rates and [Fe II]5.34μm/[Ar II]6.99μm in the deprojected 400 pc nuclear region to scale positively with both the ionized outflow rate and the estimated molecular gas temperature. We do not observe the estimated jet cavity power within the central 400 pc as strongly correlated with the ionized mass outflow rate or molecular gas temperature of the nuclear region. We take the preceding observations to suggest a higher degree of interaction between AGN outflows and the circumnuclear disk.
Publication status:
Published
Peer review status:
Peer reviewed

Actions

Access Document

Files:
Publisher copy:
10.3847/1538-4357/ae548a

Authors

More by this author
Role:
Author
ORCID:
0009-0007-6992-2555
More by this author
Role:
Author
ORCID:
0000-0002-4457-5733
More by this author
Role:
Author
ORCID:
0000-0003-4937-9077
More by this author
Role:
Author
ORCID:
0000-0003-4949-7217
More by this author
Role:
Author
ORCID:
0000-0001-7827-5758


More from this funder
Funder identifier:
10.13039/100013757
Grant:
JWST-GO-01670
More from this funder
Grant:
22-ADAP22-0173


Publisher:
American Astronomical Society
Journal:
The Astrophysical Journal More from this journal
Volume:
1002
Issue:
1
Pages:
20
Article number:
20
Publication date:
2026-04-22
Acceptance date:
2026-03-09
DOI:
EISSN:
1538-4357
ISSN:
0004637X, 0004-637X


Language:
English
Keywords:
Pubs id:
2412556
Local pid:
pubs:2412556
Source identifiers:
3973552
Deposit date:
2026-04-22
ARK identifier:
This ORA record was generated from metadata provided by an external service. It has not been edited by the ORA Team.

Terms of use


Views and Downloads






If you are the owner of this record, you can report an update to it here: Report update to this record

TO TOP