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PHANGS–JWST First Results: Mid-infrared Emission Traces Both Gas Column Density and Heating at 100 pc Scales


Abstract We compare mid-infrared (mid-IR), extinction-corrected H$\alpha$, and CO (2-1) emission at 70--160 pc resolution in the first four PHANGS-JWST targets. We report correlation strengths, intensity ratios, and power law fits relating emission in JWST's F770W, F1000W, F1130W, and F2100W bands to CO and H$\alpha$. At these scales, CO and H$\alpha$ each correlate strongly with mid-IR emission, and these correlations are each stronger than the one relating CO to H$\alpha$ emission. This reflects that mid-IR emission simultaneously acts as a dust column density tracer, leading to the good match with the molecular gas-tracing CO, and as a heating tracer, leading to the good match with the H$\alpha$. By combining mid-IR, CO, and H$\alpha$ at scales where the overall correlation between cold gas and star formation begins to break down, we are able to separate these two effects. We model the mid-IR above $I_\nu = 0.5$~MJy sr$^{-1}$ at F770W, a cut designed to select regions where the molecular gas dominates the interstellar medium (ISM) mass. This bright emission can be described to first order by a model that combines a CO-tracing component and an H$\alpha$-tracing component. The best-fitting models imply that $\sim 50\%$ of the mid-IR flux arises from molecular gas heated by the diffuse interstellar radiation field, with the remaining $\sim 50\%$ associated with bright, dusty star forming regions. We discuss differences between the F770W, F1000W, F1130W bands and the continuum dominated F2100W band and suggest next steps for using the mid-IR as an ISM tracer.
Authors Adam K. Leroy ORCID , Karin Sandström ORCID , Erik Rosolowsky ORCID , Francesco Belfiore ORCID , Alberto D. Bolatto ORCID , Yixian Cao ORCID , Eric W. Koch ORCID , E. Schinnerer ORCID , Ashley T. Barnes ORCID , Ivana Bešlić ORCID , Frank Bigiel ORCID , Guillermo A. Blanc ORCID , Jérémy Chastenet ORCID , Ness Mayker Chen ORCID , Mélanie Chevance ORCID , Ryan Chown ORCID , Enrico Congiu ORCID , Daniel A. Dale University of WyomingORCID , Oleg V. Egorov ORCID , Éric Emsellem ORCID , Cosima Eibensteiner ORCID , 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 , María J. Jiménez-Donaire ORCID , Jaeyeon Kim ORCID , Ralf S. Klessen ORCID , Kathryn Kreckel ORCID , J. M. Diederik Kruijssen ORCID , Kirsten L. Larson ORCID , Janice Lee ORCID , Rebecca C. Levy ORCID , Daizhong Liu ORCID , Laura A. Lopez ORCID , Sharon E. Meidt ORCID , E. J. Murphy ORCID , Justus Neumann ORCID , Ismael Pessa ORCID , J. Pety ORCID , Tomoka Tosaki ORCID , Amy Sardone ORCID , Jiayi Sun ORCID , David A. Thilker ORCID , A. Usero ORCID , Elizabeth J. Watkins ORCID , Cory M. Whitcomb ORCID , Thomas G. Williams ORCID
Journal Info IOP Publishing | The Astrophysical Journal Letters , vol: 944 , iss: 2 , pages: L9 - L9
Publication Date 2/1/2023
ISSN 2041-8205
TypeKeyword Image article
Open Access gold Gold Access
DOI https://doi.org/10.3847/2041-8213/acaf85
KeywordsKeyword Image Gas Sensing (Score: 0.486107)