Table 3
Mass of dust disc in V892 Tau derived at each wavelength using the methods of Section 3.3.
| Wavelength (mm) | Mdust (10-4 M⊙) | |
|---|---|---|
| Kabs ∝ Vβ 1 | κabs = κDSHARP 2 | |
| 9.8 | 6.9 ± 1.3 | 220 ± 40 |
| 8.0 | 6.8 ± 1.1 | 130 ± 20 |
| 3.0 | 4.6 ± 0.2 | 28 ± 1 |
| 1.3 | 4.8 ± 0.2 | 6.6 ± 0.3 |
| 0.9 | 5.6 ± 0.6 | 4.6 ± 0.5 |
| SED | / |  |
Notes. At each wavelength, the dust mass was derived from the values of Fout listed in Table 2 using Equation (8). The last row indicates the dust mass derived from our best-fit model described in Section 3.2. 1This column corresponds to dust masses calculated assuming powerlaw opacities. 2This column corresponds to dust masses calculated assuming DSHARP opacities averaged over the dust size distribution.
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