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Table 3
Best fit models of the disk for each individual image and for the combined fit.
Image(s) |
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νa | Ab | rinner | routerc | α | f T | id | Ωe |
(AU2) | (AU) | (AU) | (°) | (°) | |||||
lower (formal) | |||||||||
|
|||||||||
70 μm | 1.04 | 408 | 0.8 ± 0.5 |
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≥ 40 (62) | − 2 ≤ α ≤ 0 |
![]() |
≤ 60 | 120 ± 20 |
100 μm | 0.99 | 408 | 2.2 ± 1.2 |
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≥ 55 (100) | − 2 ≤ α ≤ 0 |
![]() |
≤ 60 | 110 ± 20 |
160 μm | 0.97 | 90 | 1.5 ± 0.7 |
![]() |
≥ 90 (145) | − 2 ≤ α ≤ 0 |
![]() |
40 < i < 80 | 120 ± 20 |
Combined | 1.03 | 922 | 2.3 ± 1.1 |
![]() |
≥ 60 (110) | − 2 ≤ α ≤ 0 |
![]() |
30 < i < 70 | 120 ± 20 |
Notes.
(a)
Based on the number of natural pixels (the natural pixel is ~ 3 times larger than the pixel in the images shown).
(b)
A is the total cross-sectional area of all the grains (see Sect. 5.1).
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