Core Revelations: The Star Formation and Active Galactic Nucleus Connection at the Heart of NGC 7469

We investigate the star formation–active galactic nucleus (AGN) connection in the Seyfert 1 NGC 7469 using James Webb Space Telescope mid-infrared spectroscopic integral field unit (IFU) data. We use the IFU data to generate maps of different emission lines present in the spectrum, such as the star...

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Main Authors: Léa M. Feuillet, Steve Kraemer, Marcio B. Meléndez, Travis C. Fischer, Henrique R. Schmitt, James N. Reeves, Anna Trindade Falcão
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal
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Online Access:https://doi.org/10.3847/1538-4357/adb155
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author Léa M. Feuillet
Steve Kraemer
Marcio B. Meléndez
Travis C. Fischer
Henrique R. Schmitt
James N. Reeves
Anna Trindade Falcão
author_facet Léa M. Feuillet
Steve Kraemer
Marcio B. Meléndez
Travis C. Fischer
Henrique R. Schmitt
James N. Reeves
Anna Trindade Falcão
author_sort Léa M. Feuillet
collection DOAJ
description We investigate the star formation–active galactic nucleus (AGN) connection in the Seyfert 1 NGC 7469 using James Webb Space Telescope mid-infrared spectroscopic integral field unit (IFU) data. We use the IFU data to generate maps of different emission lines present in the spectrum, such as the star formation (SF) tracer [Ne ii ] 12.81 μ m and the AGN tracer [Ne v ] 14.32 μ m. We can separate the AGN- and SF-dominated regions using spatially resolved mid-infrared diagnostic diagrams, and we further investigate the ionization sources powering each region by constructing photoionization models. We find that the previously detected eastern wind populates an intermediary region of the diagrams, between our star-forming and AGN points. Although it is possible that the star-forming ring may inherently not be uniform, this wind also coincides with a reduction in the [Ne ii ] emission in the ring, which suggests that the ionization cone intersects the ring in this direction.
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spelling doaj-art-8cc4d3de8a574a3aa6f35bb0ae81efb52025-08-20T02:09:35ZengIOP PublishingThe Astrophysical Journal1538-43572025-01-0198314910.3847/1538-4357/adb155Core Revelations: The Star Formation and Active Galactic Nucleus Connection at the Heart of NGC 7469Léa M. Feuillet0https://orcid.org/0000-0002-5718-2402Steve Kraemer1https://orcid.org/0000-0003-4073-8977Marcio B. Meléndez2https://orcid.org/0000-0001-8485-0325Travis C. Fischer3https://orcid.org/0000-0002-3365-8875Henrique R. Schmitt4https://orcid.org/0000-0003-2450-3246James N. Reeves5https://orcid.org/0000-0002-0982-0561Anna Trindade Falcão6https://orcid.org/0000-0001-8112-3464Institute for Astrophysics and Computational Sciences and Department of Physics, The Catholic University of America , Washington, DC 20064, USA ; feuilletl@cua.eduInstitute for Astrophysics and Computational Sciences and Department of Physics, The Catholic University of America , Washington, DC 20064, USA ; feuilletl@cua.eduSpace Telescope Science Institute , 3700 San Martin Drive Baltimore, MD 21218, USAAURA for ESA, Space Telescope Science Institute , 3700 San Martin Drive, Baltimore, MD 21218, USANaval Research Laboratory , Remote Sensing Division, 4555 Overlook Avenue SW, Washington, DC 20375, USAInstitute for Astrophysics and Computational Sciences and Department of Physics, The Catholic University of America , Washington, DC 20064, USA ; feuilletl@cua.eduHarvard-Smithsonian Center for Astrophysics , 60 Garden Street, Cambridge, MA 02138, USAWe investigate the star formation–active galactic nucleus (AGN) connection in the Seyfert 1 NGC 7469 using James Webb Space Telescope mid-infrared spectroscopic integral field unit (IFU) data. We use the IFU data to generate maps of different emission lines present in the spectrum, such as the star formation (SF) tracer [Ne ii ] 12.81 μ m and the AGN tracer [Ne v ] 14.32 μ m. We can separate the AGN- and SF-dominated regions using spatially resolved mid-infrared diagnostic diagrams, and we further investigate the ionization sources powering each region by constructing photoionization models. We find that the previously detected eastern wind populates an intermediary region of the diagrams, between our star-forming and AGN points. Although it is possible that the star-forming ring may inherently not be uniform, this wind also coincides with a reduction in the [Ne ii ] emission in the ring, which suggests that the ionization cone intersects the ring in this direction.https://doi.org/10.3847/1538-4357/adb155Active galaxiesStarburst galaxiesInfrared galaxiesUltraluminous infrared galaxies
spellingShingle Léa M. Feuillet
Steve Kraemer
Marcio B. Meléndez
Travis C. Fischer
Henrique R. Schmitt
James N. Reeves
Anna Trindade Falcão
Core Revelations: The Star Formation and Active Galactic Nucleus Connection at the Heart of NGC 7469
The Astrophysical Journal
Active galaxies
Starburst galaxies
Infrared galaxies
Ultraluminous infrared galaxies
title Core Revelations: The Star Formation and Active Galactic Nucleus Connection at the Heart of NGC 7469
title_full Core Revelations: The Star Formation and Active Galactic Nucleus Connection at the Heart of NGC 7469
title_fullStr Core Revelations: The Star Formation and Active Galactic Nucleus Connection at the Heart of NGC 7469
title_full_unstemmed Core Revelations: The Star Formation and Active Galactic Nucleus Connection at the Heart of NGC 7469
title_short Core Revelations: The Star Formation and Active Galactic Nucleus Connection at the Heart of NGC 7469
title_sort core revelations the star formation and active galactic nucleus connection at the heart of ngc 7469
topic Active galaxies
Starburst galaxies
Infrared galaxies
Ultraluminous infrared galaxies
url https://doi.org/10.3847/1538-4357/adb155
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