Table B.1
Parameters of our SPH simulations.
| Parameters | Value |
|---|---|
| M* [M⊙] | 1 |
| Mdisc [M⊙] | [0.01, 0.025, 0.05, 0.1, 0.15, 0.2] |
| Rin [au] | 10 |
| Rout [au] | 300 |
| Rc [au] | 100 |
| γ | 1. |
| q | 0.5 |
| αss | 0.005 |
| (H/R)c | 0.075 |
Notes. M* is the star mass and Mdisc is the disc initial mass. Rin and Rout denote the initial disc inner and outer radii. The surface density profile of Eq. 2 is parametrised by the radius of the exponential tapering Rc and the power-law index p. Here, q is the power-law index of the temperature radial profile as in Eq. 4, αss is the effective Shakura & Sunyaev (1973) viscosity, and (H/R)c is the disc aspect ratio at the reference radius Rc.
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.