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Mass-loss rates during the red supergiant phase are very poorly constrainedfrom an observational or theoretical point of view. However, they can be veryhigh, and make a massive star lose a lot of mass during this phase, influencingconsiderably the final evolution of the star: will it end as a red supergiant?Will it evolve bluewards by removing its hydrogen-rich envelope? In this paper,we briefly summarise the effects of this mass loss and of the relateduncertainties, particularly on the population of blue supergiant stars.

Mass loss of red supergiants: a key ingredient for the final evolution of massive stars