Open Access

This article has an erratum: [https://doi.org/10.1051/0004-6361/202451953e]


Fig. 8.

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Axial ratio (b/a) against stellar mass (top) and ⟨ t ⟩M (bottom) for Hα clumps (gold), F275W clumps (pink), and star-forming complexes (purple). Median lines are color-coded as the points and error bars represent interquartile regions for each b/a bin.

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