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This article has an erratum: [https://doi.org/10.1051/0004-6361/201526463e]


Fig. A.2

image

Final masses of planets as a function of initial radius r0 and initial time t0 in the disc, where Z = 1.0%, and a total disc lifetime of 5 Myr. The lines inside the plots correspond to the same meaning as the lines in Fig. 4. Clearly the formation of small planets is delayed to times after t0 = 3.5 Myr.

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