Do stars still form in molecular gas within CO-dark dwarf galaxies? - Université de Lyon
Journal Articles Monthly Notices of the Royal Astronomical Society Year : 2024

Do stars still form in molecular gas within CO-dark dwarf galaxies?

David J. Whitworth
  • Function : Author
Rowan J. Smith
  • Function : Author
Simon C. O. Glover
  • Function : Author
Robin Tress
  • Function : Author
Elizabeth J. Watkins
  • Function : Author
Jian-Cheng Feng
  • Function : Author
Ralf S. Klessen
  • Function : Author
Paul C. Clark
  • Function : Author

Abstract

In the Milky Way and other main-sequence galaxies, stars form exclusively in molecular gas, which is traced by CO emission. However, low metallicity dwarf galaxies are often 'CO-dark' in the sense that CO emission is not observable even at the high resolution and sensitivities of modern observing facilities. In this work we use ultra high-resolution simulations of four low-metalicity dwarf galaxies (which resolve star formation down to the scale of star-forming cores, 0.01 pc) combined with a time-dependent treatment of the chemistry of the interstellar medium, to investigate the star formation environment in this previously hidden regime. By generating synthetic observations of our models we show that the galaxies have high to extremely high dark gas fractions (0.13 to 1.00 dependent on beam size and conditions), yet despite this form stars. However, when examined on smaller scales, we find that the stars still form in regions dominated by molecular gas, it is simply that these are far smaller than the scale of the beam (1.5″). Thus, while stars in CO-dark dwarf galaxies form in small molecular cores like larger galaxies, their cloud-scale environment is very different.
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insu-04858878 , version 1 (30-12-2024)

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David J. Whitworth, Rowan J. Smith, Simon C. O. Glover, Robin Tress, Elizabeth J. Watkins, et al.. Do stars still form in molecular gas within CO-dark dwarf galaxies?. Monthly Notices of the Royal Astronomical Society, In press, ⟨10.1093/mnras/stae2759⟩. ⟨insu-04858878⟩
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