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arXiv · 2507.19573

Observed Timescales of Stellar Feedback in Star-Forming, Low-Mass Galaxies

Laura C. Hunter·Liese van Zee·Roger E. Cohen·Kristen B. McQuinn·Madison Markham·Justin A. Kader·Lexi N. Gault·Andrew E. Dolphin
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Abstract

Understanding the timescales of atomic gas turbulence is crucial to understanding the interplay between star formation and the interstellar medium (ISM). To investigate the timescales of turbulence low-mass galaxies ($10^{6.8} $100 Myr ago, and the HI turbulence properties, may be related to the time scales over which turbulence decays in the ISM. Additionally, the results demonstrate a possible difference in the global and local turbulence properties of low-mass galaxies.

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Laura C. Hunter, Liese van Zee, Roger E. Cohen, Kristen B. McQuinn, Madison Markham, Justin A. Kader, Lexi N. Gault, Andrew E. Dolphin. 2025-07-25. Observed Timescales of Stellar Feedback in Star-Forming, Low-Mass Galaxies. https://arxiv.org/abs/2507.19573

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