The Astrophysical Journal Letters (Jan 2023)

PHANGS–JWST First Results: Destruction of the PAH Molecules in H ii Regions Probed by JWST and MUSE

  • Oleg V. Egorov,
  • Kathryn Kreckel,
  • Karin M. Sandstrom,
  • Adam K. Leroy,
  • Simon C. O. Glover,
  • Brent Groves,
  • J. M. Diederik Kruijssen,
  • Ashley. T. Barnes,
  • Francesco Belfiore,
  • F. Bigiel,
  • Guillermo A. Blanc,
  • Médéric Boquien,
  • Yixian Cao,
  • Jérémy Chastenet,
  • Mélanie Chevance,
  • Enrico Congiu,
  • Daniel A. Dale,
  • Eric Emsellem,
  • Kathryn Grasha,
  • Ralf S. Klessen,
  • Kirsten L. Larson,
  • Daizhong Liu,
  • Eric J. Murphy,
  • Hsi-An Pan,
  • Ismael Pessa,
  • Jérôme Pety,
  • Erik Rosolowsky,
  • Fabian Scheuermann,
  • Eva Schinnerer,
  • Jessica Sutter,
  • David A. Thilker,
  • Elizabeth J. Watkins,
  • Thomas G. Williams

DOI
https://doi.org/10.3847/2041-8213/acac92
Journal volume & issue
Vol. 944, no. 2
p. L16

Abstract

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Polycyclic aromatic hydrocarbons (PAHs) play a critical role in the reprocessing of stellar radiation and balancing the heating and cooling processes in the interstellar medium but appear to be destroyed in H ii regions. However, the mechanisms driving their destruction are still not completely understood. Using PHANGS–JWST and PHANGS–MUSE observations, we investigate how the PAH fraction changes in about 1500 H ii regions across four nearby star-forming galaxies (NGC 628, NGC 1365, NGC 7496, and IC 5332). We find a strong anticorrelation between the PAH fraction and the ionization parameter (the ratio between the ionizing photon flux and the hydrogen density) of H ii regions. This relation becomes steeper for more luminous H ii regions. The metallicity of H ii regions has only a minor impact on these results in our galaxy sample. We find that the PAH fraction decreases with the H α equivalent width—a proxy for the age of the H ii regions—although this trend is much weaker than the one identified using the ionization parameter. Our results are consistent with a scenario where hydrogen-ionizing UV radiation is the dominant source of PAH destruction in star-forming regions.

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