Extended Data Fig. 1: Radial profiles of quantities describing the galactic structure of NGC 300.
From: Fast and inefficient star formation due to short-lived molecular clouds and rapid feedback
a–f, The surface densities of molecular gas, atomic gas, total gas and stars (a), the SFR surface density (b), the depletion times of molecular, atomic and total gas (c), the rotation curve (d), the Toomre Q stability parameter (e, where Q = 1 corresponds to equilibrium), and the metallicity (f).
