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The theory of radiatively driven winds successfully explains the key pointsof the stellar winds of hot massive stars. However, there is an apparentbreak-down of this paradigm at L/Lsun<5.2: the stellar wind momentum is smallerthan predicted for low luminosity early-type stars from metal poorenvironments, and there are also some Galactic examples. In this work weexplore whether magnetic fields are playing a role.

Exploring the connection of weak winds and magnetic fields