A high angular resolution view of the PAH emission in Seyfert galaxies using JWST/MRS data
García-Bernete, I.; Rigopoulou, D.; Alonso-Herrero, A.; Donnan, F.R.; Roche, P.F.; Pereira-Santaella, M.; Labiano, A.; Peralta de Arriba, L.; Izumi, T.; Ramos Almeida, C.; Shimizu, T.; Hönig, S.; García-Burillo, S.; Rosario, D.J.; Ward, M.J.; Bellocchi, E.; Hicks, E.K.S.; Fuller, L.; Packham, C.
L. Peralta de Arriba
C. Ramos Almeida
Professor Martin Ward firstname.lastname@example.org
External Examiner (PGR)
Polycyclic aromatic hydrocarbons (PAHs) are carbon-based molecules that are ubiquitous in a variety of astrophysical objects and environments. In this work we use JWST/MIRI MRS spectroscopy of three Seyferts to compare their nuclear PAH emission with that of star-forming (SF) regions. This study represents the first of its kind to use sub-arcsecond angular resolution data of local luminous Seyferts (Lbol > 1044.46 erg s−1 ) with a wide wavelength coverage (4.9–28.1 µm). We present an analysis of their nuclear PAH properties by comparing the observed ratios with PAH diagnostic model grids derived from theoretical spectra. Our results show that a suite of PAH features is present in the innermost parts of luminous Seyfert galaxies (∼0.4500 at 12 µm; in the inner ∼142–245 pc). We find that the nuclear regions of active galactic nuclei (AGN) lie at different positions of the PAH diagnostic diagrams, whereas the SF regions are concentrated around the average values of SF galaxies. In particular, we find that the nuclear PAH emission mainly originates in neutral PAHs. In contrast, PAH emission originating in the SF regions favours ionised PAH grains. The observed PAH ratios in the nuclear region of the AGN-dominated galaxy NGC 6552 indicate the presence of larger PAH molecules compared with those of the SF regions. Therefore, our results provide evidence that the AGN have a significant impact on the ionisation state (and probably the size) of the PAH grains on scales of ∼142–245 pc.
García-Bernete, I., Rigopoulou, D., Alonso-Herrero, A., Donnan, F., Roche, P., Pereira-Santaella, M., …Packham, C. (2022). A high angular resolution view of the PAH emission in Seyfert galaxies using JWST/MRS data. Astronomy & Astrophysics, 666, Article L5. https://doi.org/10.1051/0004-6361/202244806
|Journal Article Type||Article|
|Acceptance Date||Sep 20, 2022|
|Online Publication Date||Sep 30, 2022|
|Deposit Date||Mar 6, 2023|
|Publicly Available Date||Mar 6, 2023|
|Journal||Astronomy & Astrophysics|
|Peer Reviewed||Peer Reviewed|
Published Journal Article
Publisher Licence URL
Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0),<br /> which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.<br /> This article is published in open access under the Subscribe-to-Open model. Subscribe to A&A to support open access publication.
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