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arXiv · 1012.2360

Discovery of the shortest rotational period, non-degenerate, magnetic massive star by the MiMeS Collaboration

J. H. Grunhut·G. A. Wade·T. Rivinius·W. L. F. Marcolino·R. Townsend·the MiMeS Collaboration
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Abstract

We discuss the recent detection of a strong, organized magnetic field in the bright, broad-line B2V star, HR 5907, using the ESPaDOnS spectropolarimeter on the CFHT as part of the Magnetism in Massive Stars (MiMeS) survey. We find a rotational period of 0.50833 days, making it the fastest-rotating, non-degenerate magnetic star ever detected. Like the previous rapid-rotation record holder HR 7355 (also discovered by MiMeS: Oksala et al. 2010, Rivinius et al. 2010), this star shows emission line variability that is diagnostic of a structured magnetosphere.

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J. H. Grunhut, G. A. Wade, T. Rivinius, W. L. F. Marcolino, R. Townsend, the MiMeS Collaboration. 2010-12-10. Discovery of the shortest rotational period, non-degenerate, magnetic massive star by the MiMeS Collaboration. https://arxiv.org/abs/1012.2360

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