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Polar Magnetic Activity and Spin‐down on the Lower Main Sequence

  • Authors: D. L. Buzasi

Buzasi 1997 The Astrophysical Journal 484 855.

  • Provider: AAS Journals

Caption: Fig. 3.

Trajectories of rising flux tubes in the convective envelope of a star of mass 0.4 M and age 500 Myr. The paths are labeled by rotational velocity, and all begin at θ = 10°.

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