A synthesis review concluding that red supergiant mass loss is gravity-driven, metallicity-independent in rate, and bimodal, with low-mass stars keeping their mantles to core collapse and massive stars shedding them to become yellow hypergiants.
Investigating dusty red supergiant outflows in Westerlund 1 with 3D Hydrodynamic simulations
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Red Supergiant Mass Loss and Mass-Loss Rates
A synthesis review concluding that red supergiant mass loss is gravity-driven, metallicity-independent in rate, and bimodal, with low-mass stars keeping their mantles to core collapse and massive stars shedding them to become yellow hypergiants.