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We report the discovery and analysis of a very strong magnetic field in the rapidly rotating early B‐type star HR 5907, based on observations obtained as part of the Magnetism in Massive Stars (MiMeS) project. We infer a rotation period of 0.508 276+0.000 015−0.000 012 d from photometric and Hα EW measurements, making this the shortest period, non‐degenerate, magnetic massive star known to date. From...
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