Kyushu University researchers have shed new light into a critical question on how baby stars develop. Using the ALMA radio telescope in Chile, the team found that in its infancy, the protostellar disk that surrounds a baby star discharges plumes of dust, gas, and electromagnetic energy.
Researchers find baby stars discharge plume-like 'sneezes' of magnetic flux during formation retrieved 11 April 2024 from https://phys.org/news/2024-04-baby-stars-discharge-plume-magnetic.html
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