Abstract We present a large set of numerical calculations describing the rotational evolution of a solar-type star, in response to the torque exerted on it by a magnetically coupled wind emanating from its surface. We consider a situation where the internal redistribution of ...
CITATION STYLE
Charbonneau, P., & MacGregor, K. B. (1993). Angular Momentum Transport in Magnetized Stellar Radiative Zones. II. The Solar Spin-down. The Astrophysical Journal, 417, 762. https://doi.org/10.1086/173357
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