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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. 4.

A summary of model results for a range of stellar masses. In each case, the emergence latitude for a flux tube that began at θ = 10° is shown. The open crosses indicate 1.0 M stars, the open squares 0.9 M, the open triangles 0.8 M, the open circles 0.7 M, the filled squares 0.6 M, the filled triangles 0.5 M, and the filled circles 0.4 M.

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