Extended Data Fig. 3: Radial profiles of the average properties of the GMC population in NGC 300.
From: Fast and inefficient star formation due to short-lived molecular clouds and rapid feedback
a–f, The GMC radius (a), velocity dispersion (b), luminous and virial masses (c), surface density (d), molecular hydrogen number density (e) and virial parameter (f, where αvir = 1 corresponds to virial equilibrium).
