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

Whitworth, David J., Smith, Rowan J., Glover, Simon C. O., Tress, Robin, Watkins, Elizabeth J., Feng, Jian-Cheng, Brucy, Noé, Klessen, Ralf S. and Clark, Paul C. ORCID: https://orcid.org/0000-0002-4834-043X 2025. Do stars still form in molecular gas within CO-dark dwarf galaxies? Monthly Notices of the Royal Astronomical Society 536 (3) , 2936–2955. 10.1093/mnras/stae2759

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License Start date: 15 December 2024

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.

Item Type: Article
Date Type: Publication
Status: Published
Schools: Physics and Astronomy
Additional Information: License information from Publisher: LICENSE 1: URL: https://creativecommons.org/licenses/by/4.0/, Start Date: 2024-12-15
Publisher: Oxford University Press
ISSN: 0035-8711
Date of First Compliant Deposit: 8 January 2025
Date of Acceptance: 8 December 2024
Last Modified: 08 Jan 2025 10:45
URI: https://orca.cardiff.ac.uk/id/eprint/175103

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