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Linking Stellar Populations to H II Regions across Nearby Galaxies. II. Infrared Reprocessed and UV Direct Radiation Pressure in H II Regions

Authors: Debosmita Pathak, Adam K. Leroy, Todd A. Thompson, Laura A. Lopez, Ashley. T. Barnes, Daniel A. Dale, Ian Blackstone, Simon C. O. Glover, Shyam H. Menon, Jessica Sutter, Thomas G. Williams, Dalya Baron, Francesco Belfiore, Frank Bigiel, Alberto D. Bolatto, Médéric Boquien, Rupali Chandar, Mélanie Chevance, Ryan Chown, Kathryn Grasha, Brent Groves, Ralf S. Klessen, Kathryn Kreckel, Jing Li, J. Eduardo Méndez-Delgado, Erik Rosolowsky, Karin Sandstrom, Sumit K. Sarbadhicary, Jiayi Sun, Leonardo Úbeda

Debosmita Pathak et al 2025 The Astrophysical Journal 982 .

Provider: AAS Journals

Caption: Figure 9.

Here we compare ﹩{P}_{{\rm{Reprocessed}}}^{{\rm{Rad}}}﹩ (maroon), ﹩{P}_{{\rm{Direct}}}^{{\rm{Rad}}}﹩ (navy), ﹩{P}_{{\rm{Ion}}}^{{\rm{Rad}}}﹩ (green), and the Strömgren P_Therm (gray) for the full sample of H II regions. The hatched regions show the 16th–84th percentiles, and the solid lines show the median of each radiation pressure term. Variation of the pressures with ﹩{L}_{{\rm{H}}\alpha }^{{\rm{corr}}}﹩ (left panel) and R_circ (right panel) for each region is included for comparison.

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