Fig. 1
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Dust mass as a function of time for the same planets as in Fig. 1 in Savvidou & Bitsch (2023), using the standard set of parameters (Table A.1). The dashed lines show the time evolution of the optically thin dust mass and the red line shows the time evolution of the dust mass for a simulation without a planet. The dot marks the last dust mass if a planet reaches the inner edge of the disk.
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