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Fig. 4


Migration of a planet pair in the gaseous disk. Black lines trace the time evolution of the semi-major axes of the planets and the blue dashed line represents the inner magnetospheric radius rc. The four panels show simulations with a) default parameters; b) massive inner planet; c) strong stellar magnetic field and d) a light disk. Parameters are listed in Table 1. Vertical lines represent the time when the inner (t1) and the outer planet (t2) enter the cavity. We would like to note that the scale of the x-axis of panel d) is different from the others.

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