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A Two-Component Probability Distribution Function Describes the Mid-IR Emission from the Disks of Star-forming Galaxies


Abstract High-resolution JWST-MIRI images of nearby spiral galaxies reveal emission with complex substructures that trace dust heated both by massive young stars and the diffuse interstellar radiation field. We present high angular (0.″85) and physical resolution (20–80 pc) measurements of the probability distribution function (PDF) of mid-infrared (mid-IR) emission (7.7–21 μ m) from 19 nearby star-forming galaxies from the PHANGS-JWST Cycle 1 Treasury. The PDFs of mid-IR emission from the disks of all 19 galaxies consistently show two distinct components: an approximately lognormal distribution at lower intensities and a high-intensity power law component. These two components only emerge once individual star-forming regions are resolved. Comparing with locations of H ii regions identified from Very Large Telescope/MUSE H α mapping, we infer that the power-law component arises from star-forming regions and thus primarily traces dust heated by young stars. In the continuum-dominated 21 μ m band, the power law is more prominent and contains roughly half of the total flux. At 7.7–11.3 μ m, the power law is suppressed by the destruction of small grains (including PAHs) close to H ii regions, while the lognormal component tracing the dust column in diffuse regions appears more prominent. The width and shape of the lognormal diffuse emission PDFs in galactic disks remain consistent across our sample, implying a lognormal gas column density N (H) ≈ 10 21 cm −2 shaped by supersonic turbulence with typical (isothermal) turbulent Mach numbers ≈5−15. Finally, we describe how the PDFs of galactic disks are assembled from dusty H ii regions and diffuse gas and discuss how the measured PDF parameters correlate with global properties such as star formation rate and gas surface density.
Authors Debosmita Pathak ORCID , Adam K. Leroy ORCID , Todd A. Thompson ORCID , Laura A. Lopez ORCID , Francesco Belfiore ORCID , M. Boquien ORCID , Daniel A. Dale University of WyomingORCID , Simon C. O. Glover ORCID , Ralf S. Klessen ORCID , Eric W. Koch ORCID , Erik Rosolowsky ORCID , Karin Sandström ORCID , E. Schinnerer ORCID , Rowan J. Smith ORCID , Jiayi Sun ORCID , Jessica Sutter ORCID , Thomas G. Williams ORCID , Frank Bigiel ORCID , Yixian Cao ORCID , Jérémy Chastenet ORCID , Mélanie Chevance ORCID , Ryan Chown ORCID , Éric Emsellem ORCID , Christopher M. Faesi ORCID , Kirsten L. Larson ORCID , M. Boquien ORCID , Sharon E. Meidt ORCID , Eve C. Ostriker ORCID , Lise Ramambason ORCID , Sumit K. Sarbadhicary ORCID , David A. Thilker ORCID
Journal Info Institute of Physics | The Astronomical Journal , vol: 167 , iss: 1 , pages: 39 - 39
Publication Date 12/29/2023
ISSN 0004-6256
TypeKeyword Image article
Open Access gold Gold Access
DOI https://doi.org/10.3847/1538-3881/ad110d
KeywordsKeyword Image High-Temperature Molecular Spectroscopy (Score: 0.479793)