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

  • Authors: Debosmita Pathak, Adam K. Leroy, Todd A. Thompson, Laura A. Lopez, Francesco Belfiore, Médéric Boquien, Daniel A. Dale, Simon C. O. Glover, Ralf S. Klessen, Eric W. Koch, Erik Rosolowsky, Karin M. Sandstrom, Eva Schinnerer, Rowan Smith, Jiayi Sun, Jessica Sutter, Thomas G. Williams, Frank Bigiel, Yixian Cao, Jérémy Chastenet, Mélanie Chevance, Ryan Chown, Eric Emsellem, Christopher M. Faesi, Kirsten L. Larson, Janice C. Lee, Sharon Meidt, Eve C. Ostriker, Lise Ramambason, Sumit K. Sarbadhicary, David A. Thilker

Debosmita Pathak et al 2024 The Astronomical Journal 167 .

  • Provider: AAS Journals

Caption: Figure 14.

NGC 1566 at 21 μm with all VLT/MUSE-identified H II regions outlined in blue (top), with the corresponding PDF (middle) and log-PDF in intensity (bottom). A few of the largest H II regions in NGC 1566 are highlighted in green. The overall pdf and log-PDF of intensities at 21 μm (black), from all H II regions (blue), and each of the highlighted individual H II regions (green) are shown for comparison.

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