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Discovery of the most rapidly-rotating, non-degenerate, magnetic massive star by the MiMeS collaboration

We discuss the recent detection of a strong, organized magnetic field in the bright, broad-line B2V star, HD 142184, 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.

preprint2010arXivOpen access
J. H. GrunhutG. A. WadeT. RiviniusW. L. F. MarcolinoR. H. D. Townsendthe MiMeS Collaboration
astro-ph.SR
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J. H. GrunhutG. A. WadeT. RiviniusW. L. F. MarcolinoR. H. D. Townsendthe MiMeS Collaboration

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