Magnetic fields and internal mixing of main sequence B stars

C.P. Folsom; G.A. Wade; J.D. Landstreet; J. Grunhut; V. Petit

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Magnetic fields and internal mixing of main sequence B stars

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arxiv 1408.0383 v1 pith:SKEH63K2 submitted 2014-08-02 astro-ph.SR

G.A. Wade , C.P. Folsom , J. Grunhut , J.D. Landstreet , V. Petit This is my paper · ORCID

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We have obtained high-quality magnetic field measurements of 19 sharp-lined B-type stars with precisely-measured N/C abundance ratios. Our primary goal is to test the idea that a magnetic field may explain extra drag (through the wind) on the surface rotation, thus producing more internal shear and mixing, and thus could provide an explanation for the appearance of slowly rotating N-rich main sequence B stars.

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