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This article has an erratum: [https://doi.org/10.1051/0004-6361/201628955e]


Fig. 11

image

Migration efficiency for Earth-mass planets for MRI-inactive cases with Σ-dependent torque (red for strong DW and blue for weak DW of Table 2) at t = 106 yr (corresponding to the solid red and blue lines in Fig. 5) in comparison to the MRI-inactive no DW case (black). CI > 0 means outward migration.

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