Free Access
Table 2
Adopted parameter distributions for the population synthesis study in Sect. 4.
| Parameter | Description | |
|---|---|---|
| disk model | viscously heated + stellar irradiation | |
| Ṁg0 [M⊙ yr−1] |  , μ is from Eq. (1) and σ = 0.3 |
|
| Mp0[ M⊕] | Eq. (14), self-gravitating disk (γ = 1) | |
| non-self-gravitating disk (γ ≠ 1) | ||
| r0 [AU] | Scenario A: the ice line | |
| Scenario B: logU(0.01, 10) | ||
| t0 [Myr] | U(0.1, 0.5) | |
| M⋆ [ M⊙] | logU(0.01, 0.1) | |
| Z⋆ | U(−0.5, 0.5) | |
| Pebble size | one millimeter |
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.