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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 7.

The distribution of ﹩{P}_{{\rm{Direct}}}^{{\rm{Rad}}}/{P}_{{\rm{Ion}}}^{{\rm{Rad}}}﹩ for our target regions split by local galactic environment. The light-blue line shows the median value of 〈τUV〉 (right y-axis) for the regions in each bin. The vertical dashed line indicates where ﹩{P}_{{\rm{Direct}}}^{{\rm{Rad}}}={P}_{{\rm{Ion}}}^{{\rm{Rad}}}﹩. This corresponds to 〈τUV〉 = 0.27.

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