Having studied similar helium-rich stars before, Shenar thought magnetic fields could crack the case. Indeed, magnetic fields are known to influence the behaviour of stars and could explain why traditional models failed to describe HD 45166, which is located about 3000 light-years away in the constellation Monoceros. “I remember having a Eureka moment while reading the literature: ‘What if the star is magnetic?’,” says Shenar, who is currently based at the Centre for Astrobiology in Madrid, Spain.
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