A Two-Component Probability Distribution Function Describes the Mid-IR Emission from the Disks of Star-forming GalaxiesDOI: info:10.3847/1538-3881/ad110dv. 167IOP39
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. et al. 2024. "A Two-Component Probability Distribution Function Describes the Mid-IR Emission from the Disks of Star-forming Galaxies." The Astronomical Journal, 167 39. https://doi.org/10.3847/1538-3881/ad110d.