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Stopping inward planetary migration by a toroidal magnetic field

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Academic year: 2021

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Figure

Figure 1. Distance of the outer turning points (thin solid lines) and magnetic resonance (thick bold lines) to corotation in units of H ≡ c / versus m for β = 0.1 (upper plot), 1 (middle plot) and 10 (lower plot) and for H / r = 0.03.
Figure 2. Results for B = 0, d 1 ≡ d ln / d ln r = 0, c / (r p  p ) = 0.03 (c 1 = 0) and m = 10
Figure 3. Results for B = 0: ˜ W m  versus r / r p for d 1 = 0, c / (r p  p ) = 0.03 (c 1 = 0), b 1 = 2, β = const = 1 and m = 10
Figure 4. Torque density ˜ T m , D versus r / r p for the same parameters as in Fig. 3
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