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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 17.

The PDFs of gas column density N(H) in diffuse regions (hatched red) derived from 7.7 μm intensities (Equations (13) and (14)) for each galaxy. Lognormal fits to each of the PDFs with the fit means are overlaid in black for comparison. The best-fit lognormal mean N(H) (μ N ) and dispersion (σ N ) are included, as in Table 2.

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