Figure 19.
The field strength predicted at the surface of massive stars. The prediction assumes an equipartition dynamo in the convective layer and a B∝ρ2/3 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].
