FEAST: Feedback in emerging extragAlactic star ClusTers: JWST spots polycyclic aromatic hydrocarbon destruction in NGC 628 during the emerging phase of star formation

Pedrini, Alex, Adamo, Angela, Calzetti, Daniela, Bik, Arjan, Gregg, Benjamin, Linden, Sean T., Bajaj, Varun, Ryon, Jenna E., Ali, Ahmad A., Bortolini, Giacomo, Correnti, Matteo, Elmegreen, Bruce G., Elmegreen, Debra Meloy, Gallagher, John S., Grasha, Kathryn, Gutermuth, Robert A., Johnson, Kelsey E., Melinder, Jens, Messa, Matteo, Östlin, Göran, Sabbi, Elena, Smith, Linda J., Tosi, Monica and Faustino Vieira, Helena 2024. FEAST: Feedback in emerging extragAlactic star ClusTers: JWST spots polycyclic aromatic hydrocarbon destruction in NGC 628 during the emerging phase of star formation. The Astrophysical Journal 971 , 32. 10.3847/1538-4357/ad534d

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Abstract

We investigate the emergence phase of young star clusters in the nearby spiral galaxy NGC 628. We use JWST NIRCam and MIRI observations to create spatially resolved maps of the Paα 1.87 μm and Brα 4.05 μm hydrogen recombination lines, as well as 3.3 and 7.7 μm emission from polycyclic aromatic hydrocarbons (PAHs). We extract 953 compact H ii regions and analyze the PAH emission and morphology at ∼10 pc scales in the associated photodissociation regions. While H ii regions remain compact, radial profiles help us to define three PAH morphological classes: compact (∼42%), extended (∼34%), and open (∼24%). The majority of compact and extended PAH morphologies are associated with very young star clusters (<5 Myr), while open PAH morphologies are mainly associated with star clusters older than 3 Myr. We observe a general decrease in the 3.3 and 7.7 μm PAH band emission as a function of cluster age, while their ratio remains constant with age out to 10 Myr and morphological class. The recovered PAH3.3μm/PAH7.7μm ratio is lower than values reported in the literature for reference models that consider neutral and ionized PAH populations and analyses conducted at galactic physical scales. The 3.3 and 7.7 μm bands are typically associated with neutral and ionized PAHs, respectively. While we expected neutral PAHs to be suppressed in proximity to an ionizing source, the constant PAH3.3μm/PAH7.7μm ratio would indicate that both families of molecules disrupt at similar rates in proximity to H ii regions.

Item Type:	Article
Date Type:	Published Online
Status:	Published
Schools:	Physics and Astronomy
Additional Information:	License information from Publisher: LICENSE 1: URL: http://creativecommons.org/licenses/by/4.0/, Type: cc-by. This article has an Erratum: Alex Pedrini et al 2024 ApJ 973 67. 10.3847/1538-4357/ad74ee
Publisher:	American Astronomical Society
ISSN:	0004-637X
Related URLs:	https://doi.org/10.3847/1538-4357/ad74ee
Date of First Compliant Deposit:	6 August 2024
Date of Acceptance:	31 May 2024
Last Modified:	01 Oct 2024 08:19
URI:	https://orca.cardiff.ac.uk/id/eprint/171172

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