In the Magellanic Clouds, researchers have detected magnetic fields in three massive and hot stars for the first time. This discovery is significant because it provides a unique opportunity to study stars in active formation and the upper limit of mass that one can have and remain stable. Magnetism is considered a key component in the evolution of massive stars, with far-reaching impacts on their ultimate fate. These stars, with more than eight solar masses at the beginning, leave behind neutron stars and black holes at the end of their evolution. Gravitational-wave observatories have captured spectacular mergers of these compact remnant systems, while theoretical studies propose a magnetic mechanism for the explosion of massive stars, relevant to gamma-ray bursts, X-ray flares, and supernovae. Studies of magnetic fields in massive stars in galaxies with young stellar populations provide crucial information on the role of magnetic fields in star formation in the early universe with star-forming gas not contaminated by metals.
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