Open Access

Fig. 4


Column density for our MHD simulations (2563), with feedback by supernovae and H II regions, at 80 Myrs. For each plane, there are two rows: the first one does not display sink particles, but the second one does, each one representing a star cluster (the colours are random). Left panel: Vshear = 28 km s−1 kpc−1. Right panel: Vshear = 56 km s−1 kpc−1.

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