Fig. 14
For aB5 V star model with a magnetic field of B = 1 kG for inward directed Lorentz force. Right panels: log Ni vs. cos (θ) (θ, co-latitudinal angle) are plotted for H II at log τ = 0.5 and for He I at log τ = − 1.0. Left panels: the stellar discs are represented by the corresponding elements at the same depths in false colors.
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