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

Figure 19.

Figure 19.

The field strength predicted at the surface of massive stars. The prediction assumes an equipartition dynamo in the convective layer and a Bρ2/3 dependence in the overlying radiative layer. Also shown are the X-ray luminosities measured in a number of stars: there does seem to be some connection between subsurface convection and X-ray emission. The dotted lines are evolutionary tracks of stars of various initial masses. From Cantiello & Braithwaite [202].