Magnetic transport of angular momentum in rotating massive star models reproduces observed surface boron abundances, while purely hydrodynamic models destroy too much boron in fast rotators.
W., Eggenberger , P., & Hirschi , R
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Impact of the Tayler magnetic instability on the surface abundance of boron in massive stars
Magnetic transport of angular momentum in rotating massive star models reproduces observed surface boron abundances, while purely hydrodynamic models destroy too much boron in fast rotators.