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Fig. 3

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Solid lines displaying the median value of the bar radius in kiloparsecs vs. stellar mass for TNG50 at ɀ = 0.0, ɀ = 0.5, and ɀ = 1.0 and for the observed CALIFA+MaNGA sample at ɀ ≃ 0.0. We have included 20 additional galaxies from CALIFA and MaNGA that do not meet the condition ΔΩp/Ωp ≤ 0.5 but satisfy ΔRbar/Rbar ≤ 0.5. The shaded areas give the 32th– 68th percentile. We only display mass bins that include more than five galaxies. We plot the same regions for other similar figures in this paper.

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