MICONIC: JWST/MIRI-MRS reveals heavily reprocessed PAH emission in the circum-nuclear disc of Centaurus A
L. Pantoni, M. Baes, L. Decin, P. Guillard, A. Alonso Herrero, L. Evangelista, L. Hermosa Mu\~noz, I. Garc\'ia-Bernete, F. Donnan, V. Buiten, S. Garcia-Burillo, G. Wright, L. Colina, T. B\"oker, G. \"Ostlin, D. Dicken, A. Labiano, D. Rouan, P. van der Werf, A. Eckart

TL;DR
This study uses JWST/MIRI-MRS observations to analyze PAH emission in Centaurus A's central region, revealing spatial variations, processed PAH populations, and evidence of shocks and destruction near the nucleus.
Contribution
First spatially resolved analysis of PAHs in Centaurus A's nucleus using JWST data, highlighting processed PAH populations and environmental effects.
Findings
PAH emission forms a ring-like structure with localized enhancements.
A PAH-deficient region shows signs of shocks and partial destruction.
PAH ratios indicate processed, open-structured PAH populations.
Abstract
Polycyclic aromatic hydrocarbons (PAHs) are key dust components in galaxies and play a fundamental role in the physics of the interstellar medium (ISM), yet their response to AGN feedback remains debated. We present a spatially resolved analysis of PAHs in the central ( pc) of Centaurus A. We use JWST/MIRI-MRS observations at 5-28 m from the MIRI European consortium GTO program MICONIC, with angular resolution of (about 6-17 pc). We derive PAH moment-0 maps via local continuum subtraction and extract one-dimensional spectra from five regions of interest, including the nucleus, the circumnuclear disc, and a PAH-deficient region. The spectra are decomposed into continuum, emission lines, and PAHs to measure feature intensities and equivalent widths (EWs). PAH emission is primarily…
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Taxonomy
TopicsAstrophysics and Star Formation Studies · Galaxies: Formation, Evolution, Phenomena · Astronomy and Astrophysical Research
