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Observed Timescales of Stellar Feedback in Star-Forming, Low-Mass Galaxies
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Observed Timescales of Stellar Feedback in Star-Forming, Low-Mass Galaxies
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Paper
Observed Timescales of Stellar Feedback in Star-Forming, Low-Mass Galaxies
2025
Overview
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.
Publisher
Cornell University Library, arXiv.org
