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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 3.

Left panel: the distribution of Hα attenuation, A_Hα, from VLT-MUSE (Section 2.1) in our sample of H II regions, colored by local environment as in Figure 2. The corresponding optical depth at 21 μm, τ_21μm, converted from A_Hα using the G23 extinction law (Table 2), is included as an alternate x-axis. Right panel: corresponding ﹩{L}_{{\rm{H}}\alpha }^{{\rm{corr}}}﹩-weighted histograms, capturing how the Hα luminosity is distributed across regions of different attenuation.

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