Fig. 15
Migration rate of a Jupiter mass planet normalized by the viscous accretion velocity. Apart from the different y-axis the plot is similar to Fig. 13. The horizontal line corresponds to 
. The dashed line shows a fit of Duffell et al. (2014), but they used constant viscosity equal to α = 0.01 at r = 5.2 au, so their fit is normalized with 
for that α.
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