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Table 3

Gaussian fit results of the simulated dust rings for all Stokes numbers, St.

a[mm] St wring1 [au] wring2 [au] rring1 [au] rring2 [au] Mring1 [Mearth] Mring2 [Mearth]
0.2 1.3 × 10−3 4.09 ± 0.09 10.5 ± 0.17 62.26 ± 0.09 100.18 ± 0.16 2.1 1.9
0.4 2.6 × 10−3 3.13 ± 0.08 7.10 ± 0.09 62.05 ± 0.08 99.90 ± 0.09 2.9 2.9
0.7 5.0 × 10−3 2.27 ± 0.07 4.80 ± 0.04 61.90 ± 0.07 99.25 ± 0.04 4.0 4.7
1.4 9.6 × 10−3 1.68 ± 0.05 3.34 ± 0.01 61.86 ± 0.05 98.87 ± 0.01 5.5 8.0
2.6 1.9 × 10−2 1.28 ± 0.04 2.37 ± 0.01 61.89 ± 0.04 98.69 ± 0.01 7.9 12.3
5.1 3.6 × 10−2 1.00 ± 0.03 1.76 ± 0.01 61.92 ± 0.03 98.67 ± 0.01 11.5 17.0
9.9 6.9 × 10−2 0.80 ± 0.03 1.33 ± 0.01 61.93 ± 0.03 98.67 ± 0.01 17.3 22.2
19.1 1.3 × 10−1 0.64 ± 0.02 1.01 ± 0.01 61.94 ± 0.02 98.66 ± 0.01 28.0 26.9
Sum (high mass model) 79.3 95.9
Sum (low mass model) 11.4 13.8

Notes. Ring widths are denoted by wring1,2 whereas the ring position is labeled rring1,2. The dust size individual mass trapped in the rings and the total mass are shown in the last two columns.

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