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NGC 2366 T op RowHimoment maps from VLA observations Left: Hicolumn density in 10 21 hydrogen atoms cm−2, Center: Hivelocity map with isovelocity contours spaces every 10 km s −1, Right: Hivelocity dispersion map with isovelocity contours a · 2000

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

astro-ph.GA · 2025-07-25 · conditional · novelty 5.0

In 26 low-mass galaxies, atomic gas turbulence correlates most strongly with star formation 100-500 million years ago, indicating a long-lived coupling between stellar feedback and the interstellar medium.

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Observed Timescales of Stellar Feedback in Star-Forming, Low-Mass Galaxies astro-ph.GA · 2025-07-25 · conditional · none · ref 3
In 26 low-mass galaxies, atomic gas turbulence correlates most strongly with star formation 100-500 million years ago, indicating a long-lived coupling between stellar feedback and the interstellar medium.

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