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

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

doi:10.3847/1538-3881/ad110d

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

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Cao, Yixian
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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Pathak, D., Leroy, A. K., Thompson, T. A., Lopez, L. A., Belfiore, F., Boquien, M., et al. (2023). A Two-Component Probability Distribution Function Describes the Mid-IR Emission from the Disks of Star-forming Galaxies. The Astronomical Journal, 167(1): 39. doi:10.3847/1538-3881/ad110d.

Cite as: https://hdl.handle.net/21.11116/0000-000E-AA0F-3

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