CORDIS Project
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This project aims to enhance our understanding of massive stars by developing new models for their radiation-driven winds. By improving predictions of mass loss and its effects on stellar evolution, the research seeks to clarify the life cycles and ultimate fates of these stars.
Across our Universe, the dynamics and chemical evolution of spiral galaxies like the Milky Way are primarily controlled by the lives and deaths of stars with masses many times that of the Sun.
But the evolution of these massive stars is, in turn, highly regulated by the huge amounts of mass lost from their surfaces, by means of powerful starlight-driven winds.
These stellar winds critically determine how such massive stars evolve through their lives, and how they finally die in giant supernova e…
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