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This article has an erratum: [https://doi.org/10.1051/0004-6361/202553939e]


Fig. B.1.

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Comparison of the clump distribution in the inner 10 kpc of our fiducial MHD simulation at t = 960 Myr with three different method. The blue and orange curves shows the distribution of the clumps with yt (Turk et al. 2011) based on density and temperature criteria. The red curve indicates the clump distribution using Scipy’s ndimage (Virtanen et al. 2020), and is comparable to the method used in (Gronke et al. 2022) and Das & Gronke (2024). The inclination of a power law of slope α ∼ −0.6 is indicated for comparison.

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