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PHANGS–JWST First Results: Tracing the Diffuse Interstellar Medium with JWST Imaging of Polycyclic Aromatic Hydrocarbon Emission in Nearby Galaxies


Abstract JWST observations of polycyclic aromatic hydrocarbon (PAH) emission provide some of the deepest and highest resolution views of the cold interstellar medium (ISM) in nearby galaxies. If PAHs are well mixed with the atomic and molecular gas and illuminated by the average diffuse interstellar radiation field, PAH emission may provide an approximately linear, high resolution, high sensitivity tracer of diffuse gas surface density. We present a pilot study that explores using PAH emission in this way based on MIRI observations of IC 5332, NGC 628, NGC 1365, and NGC 7496 from the PHANGS-JWST Treasury. Using scaling relationships calibrated in Leroy et al. (2022), scaled F1130W provides 10--40 pc resolution and 3$\sigma$ sensitivity of $\Sigma_{\rm gas} \sim 2$ M$_\odot$ pc$^{-2}$. We characterize the surface densities of structures seen at $< 7$ M$_\odot$ pc$^{-2}$ in our targets, where we expect the gas to be HI-dominated. We highlight the existence of filaments, inter-arm emission, and holes in the diffuse ISM at these low surface densities. Below $\sim 10$ M$_\odot$ pc$^{-2}$ for NGC 628, NGC 1365, and NGC 7496 the gas distribution shows a ``Swiss cheese''-like topology due to holes and bubbles pervading the relatively smooth distribution of diffuse ISM. Comparing to recent galaxy simulations, we observe similar topology for the low surface density gas, though with notable variations between simulations with different setups and resolution. Such a comparison of high resolution, low surface density gas with simulations is not possible with existing atomic and molecular gas maps, highlighting the unique power of JWST maps of PAH emission.
Authors Karin Sandström ORCID , Eric W. Koch ORCID , Adam K. Leroy ORCID , Erik Rosolowsky ORCID , Éric Emsellem ORCID , Rowan J. Smith ORCID , Oleg V. Egorov ORCID , Thomas G. Williams ORCID , Kirsten L. Larson ORCID , Janice Lee ORCID , E. Schinnerer ORCID , David A. Thilker ORCID , Ashley T. Barnes ORCID , Francesco Belfiore ORCID , Frank Bigiel ORCID , Guillermo A. Blanc ORCID , Alberto D. Bolatto ORCID , M. Boquien ORCID , Yixian Cao ORCID , Jérémy Chastenet ORCID , Mélanie Chevance ORCID , I-Da Chiang ORCID , Daniel A. Dale University of WyomingORCID , Christopher M. Faesi ORCID , Simon C. O. Glover ORCID , Kathryn Grasha ORCID , Brent Groves ORCID , Hamid Hassani ORCID , Jonathan D. Henshaw ORCID , Annie Hughes ORCID , Jaeyeon Kim ORCID , Ralf S. Klessen ORCID , Kathryn Kreckel ORCID , J. M. Diederik Kruijssen ORCID , Laura A. Lopez ORCID , Daizhong Liu ORCID , Sharon E. Meidt ORCID , E. J. Murphy ORCID , Hsi-An Pan ORCID , Miguel Querejeta ORCID , Tomoka Tosaki ORCID , Amy Sardone ORCID , Mattia C. Sormani ORCID , Jessica Sutter ORCID , A. Usero ORCID , Elizabeth J. Watkins ORCID
Journal Info IOP Publishing | The Astrophysical Journal Letters , vol: 944 , iss: 2 , pages: L8 - L8
Publication Date 2/1/2023
ISSN 2041-8205
TypeKeyword Image article
Open Access gold Gold Access
DOI https://doi.org/10.3847/2041-8213/aca972
KeywordsKeyword Image Interstellar Medium (Score: 0.47753)