Table 1
Masses, truncation radius, and their uncertainties extracted from fitting hydrodynamical rotation curves with the model of Eq. (5).
| Sims | Md (M⊙) | ΔMd/Md | Rc (au) | ΔRc/Rc |
|---|---|---|---|---|
| md0.2 | 0.19 | 0.05 | 119 | 0.19 |
| md0.15 | 0.14 | 0.06 | 113 | 0.13 |
| md0.1 | 0.1 | 0. | 106 | 0.06 |
| md0.05 | 0.05 | 0. | 94 | 0.06 |
| md0.025 | 0.028 | 0.12 | 92 | 0.08 |
| md0.01 | 0.017 | 0.7 | 86 | 0.14 |
Notes. Disc masses are all recovered with an accuracy of ~5–12% for all disc-to-star mass ratios [0.2, 0.15, 0.1, 0.05, 0.025, 0.01], except for the extreme case 0.01. The star mass 1 M⊙ is always recovered (0.98–0.99 M⊙). The input value for the truncation radius (100 au) is recovered with an accuracy of ~6–20%.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.