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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 13.

Comparing two methods for re-scaling MIRI fluxes from MUSE regions to HST for the  ∼7000 H II regions with full HST, MUSE, and JWST-MIRI coverage, colored by local environment. The x-axis scales MIRI fluxes directly by the same proportion that MUSE Hα fluxes are scaled relative to HST Hα fluxes. The y-axis calculates the total flux associated with a point source with peak intensity corresponding to the brightest pixel in each region, with a local background subtraction in each region, at ﹩0\mathop{.}\limits^{^{\prime\prime} }9﹩ resolution.

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