The Revolution Revolution: magnetic morphology driven spin-down.
2018
Observations of young
open clustersshow a
bimodaldistribution of
rotation periodsthat has been difficult to explain with existing
stellarspin-down models. Detailed MHD
stellar windsimulations have demonstrated that surface magnetic field morphology has a strong influence on wind-driven angular momentum loss. Observations suggest that faster rotating stars store a larger fraction of their magnetic flux in higher-order multipolar components of the magnetic field. In this work, we present a new model for
stellarspin-down that, for the first time, accounts for the
stellarsurface magnetic field configuration. We show how a magnetic complexity that evolves from complex toward simple configurations as a star spins down can explain the salient features of
stellar rotationevolution, including the
bimodaldistribution of both slow and fast rotators seen in young
open clusters.
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