Fig. 1
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Evolution of the stellar feedback over 1 Myr in a homogeneous ISM. First row: Density slices without cooling. Second row: Density slices with cooling. Third row: Mach number with cooling. Timestamps from left to right: 10kyr, 103 kyr, 298 kyr, 1.003 Myr. The striations aligned with the Cartesian axes visible at 1 Myr are numerical artefacts due to the stretching of the grid.
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