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The MagneticYSOs project investigates the role of magnetic fields in star formation, focusing on the dynamics of protostellar structures. It combines observational data with simulations to address the angular momentum problem critical to understanding star and planet formation.
Rotation and angular momentum transport play a critical role in the formation and evolution of astrophysical objects, including the fundamental bricks of astrophysical structures: stars.
Stars like our Sun form when rotating dense cores, in the interstellar medium, collapse until they eventually reach temperatures at which nuclear fusion begins; while planets, including the Earth, form in the rotationally supported disks around these same young stars.
One of the major challenges of modern astrop…
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