CORDIS Project
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This project investigates the impact of magnetic fields on the mass-loss processes of stars, particularly those similar to the Sun. By combining observations with theoretical models, it aims to clarify how these fields influence the expulsion of materials that contribute to the formation of stars and planets.
The study of the processes governing the end of the life of stars such as our Sun are of fundamental importance.
During the final stages of their lives, stars undergo extreme mass-loss in which they expel large amounts of dust, atoms and molecules into the interstellar environment.
This material is one of the main sources of the heavy elements essential for further formation of stars, planets and even life.
As the expelled dust is responsible for much of the emission seen from young galaxies at…
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