Shocked, heated, and now resolved: H <sub>2</sub> excitation in the low-luminosity AGN at M58 core with JWST

We present JWST NIRSpec and MIRI MRS observations of the central kiloparsec of M58 (NGC 4579), a nearby galaxy hosting a low-luminosity AGN (LLAGN; L bol ∼ 10 42 erg s −1 ) with a low-power jet. These data provide an unprecedented view of the warm molecular gas phase and reveal clear signatures of feedback. We detect 44 H 2 lines, including bright pure rotational lines (S(1)–S(18)) and rovibrational lines up to ν = 2, probing a wide range of excitation conditions. Excitation diagrams show that rotational lines follow a power-law temperature distribution with an exponential cutoff, consistent with heating by low-velocity shocks. H 2 rovibrational lines deviate from thermal models primarily because of sub-thermal excitation at low density. Additionally, there may be a 10% contribution powered by AGN X-ray photons in the nucleus. The dust lanes associated with the spiral inflow appear dynamically undisturbed but show signs of shock heating, while the inner ∼200 pc exhibits turbulent kinematics produced by outflowing molecular gas. These results reveal the subtle yet measurable impact of LLAGN feedback on the interstellar medium, demonstrating that even weak, vertically oriented jets and low radiative accretion rates can perturb molecular gas and regulate nuclear reservoirs. This study highlights JWST’s transformative ability to uncover hidden modes of AGN feedback.

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Journal
Astronomy and Astrophysics
Published
2025-12-01
DOI
https://doi.org/10.1051/0004-6361/202556565
Primary Topic
Astrophysics and Star Formation Studies
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article
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article

Shocked, heated, and now resolved: H 2 excitation in the low-luminosity AGN at M58 core with JWST

G. Cresci, V. Reynaldi, E. Bertola, Patrick Ogle et al.
Astronomy and Astrophysics
Astrophysics and Star Formation Studies
article

Shocked, heated, and now resolved: H 2 excitation in the low-luminosity AGN at M58 core with JWST

G. Cresci, V. Reynaldi, E. Bertola, Patrick Ogle, S. García‐Burillo, M. V. Zanchettin, I. E. López, R. Michael Rich, R. D. Baldi, B. Sebastian, A. Marconi, J. A. Fernández-Ontiveros, M. Brusa, Tatiana M. Rodríguez
article en

Abstract

We present JWST NIRSpec and MIRI MRS observations of the central kiloparsec of M58 (NGC 4579), a nearby galaxy hosting a low-luminosity AGN (LLAGN; L bol ∼ 10 42 erg s −1 ) with a low-power jet. These data provide an unprecedented view of the warm molecular gas phase and reveal clear signatures of feedback. We detect 44 H 2 lines, including bright pure rotational lines (S(1)–S(18)) and rovibrational lines up to ν = 2, probing a wide range of excitation conditions. Excitation diagrams show that rotational lines follow a power-law temperature distribution with an exponential cutoff, consistent with heating by low-velocity shocks. H 2 rovibrational lines deviate from thermal models primarily because of sub-thermal excitation at low density. Additionally, there may be a 10% contribution powered by AGN X-ray photons in the nucleus. The dust lanes associated with the spiral inflow appear dynamically undisturbed but show signs of shock heating, while the inner ∼200 pc exhibits turbulent kinematics produced by outflowing molecular gas. These results reveal the subtle yet measurable impact of LLAGN feedback on the interstellar medium, demonstrating that even weak, vertically oriented jets and low radiative accretion rates can perturb molecular gas and regulate nuclear reservoirs. This study highlights JWST’s transformative ability to uncover hidden modes of AGN feedback.

Astronomy and AstrophysicsVol. 704
Space Telescope Science Institute (US), Consejo Nacional de Investigaciones Científicas y Técnicas (AR), University of California, Los Angeles (US), University of Cologne (DE), Arcetri Astrophysical Observatory (IT), Istituto di Radioastronomia di Bologna (IT), Université Bourgogne Franche-Comté (FR), Centro de Estudios de Física del Cosmos de Aragón (ES), Spanish National Observatory (ES), Osservatorio di Astrofisica e Scienza dello Spazio, University of Florence (IT), Universidad Nacional de La Plata (AR), University of Bologna (IT)
Openalex Percentile: Top 74%
Astrophysics and Star Formation Studies
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