Table 1
Summary of disk models.
| Model |  |
 |
Energetics | Comments |
|---|---|---|---|---|
| disk0 | – | – | – | Power-law |
| disk1 | Active | Eq. (2) | Strong | Standard |
| disk2 | Inactive | Eq. (2) | Strong | Standard |
| disk3 | Active | Eq. (2) | Weak | – |
| disk4 | Active | 10−4 | Strong | – |
| disk5 | Inactive | Eq. (2) | Weak | – |
| disk6 | Inactive | 10−4 | Strong | – |
| disk7 | Active | Eq. (2) | Strong | t0 = 0 yr |
| disk8 | Active | Eq. (2) | Strong | t0 = 1 Myr |
| disk9 | Inactive | Eq. (2) | Strong | t0 = 0 yr |
| disk10 | Inactive | Eq. (2) | Strong | t0 = 1 Myr |
Notes. The first column gives the model name, followed by the parameter for effective turbulent viscosity
and the angular momentum loss due to the wind torque 
. The fourth column indicates the regime which is introduced by Suzuki et al. (2016) and constrains the parameter Cw. The evolution of gas surface density is shown in Fig. 1 for disk0–disk2 models and in Fig. A.1 for disk3–disk10 models.
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