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. 2017 Feb 22;4(2):160271. doi: 10.1098/rsos.160271

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© 2017 The Authors.

Published by the Royal Society under the terms of the Creative Commons Attribution License http://creativecommons.org/licenses/by/4.0/, which permits unrestricted use, provided the original author and source are credited.

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Figure 10. — A typical non-axisymmetric equilibrium as found in simulations, viewed from both sides of the star. This corresponds qualitatively to those observed on stars such as τ Sco (see figure 7). Figure from Braithwaite [93].