Effects of an outflow in the redistribution of dust. Left: Thermal pressure driven outflow launched during low-mass star and disk formation. The transient outflow seen in a 2D radiative hydrodynamic simulation lifts well-coupled dust up to 100 μm. The color shows the rotational and thermal pressure support within the collapsing protostellar core and the dashed white line indicates the protostellar disk radius. The figure is reproduced from Bhandare et al. (2024). Right: Schematic of a protostar–disk–outflow system from a 3D MHD simulation indicating the recycling of dust via outflows. This figure is reproduced from Tsukamoto et al. (2021).