Table 1.
Main parameters.
| Run name | ρ0(g cm−3) | ṁacc(ṁEdd) | sin | sout | p | A(%) | Radiative cooling |
|---|---|---|---|---|---|---|---|
| R22 | 10−22 | 1.7 × 10−6 | 1.64 | 1.94 | 0.05 | 62.00% | ON |
| R23 | 10−23 | 3.9 × 10−7 | 1.29 | 1.68 | 0.23 | 58.17% | ON |
| R24 | 10−24 | 9.0 × 10−8 | 0.86 | 1.35 | 0.37 | 55.60% | ON |
| N24 | 10−24 | 1.3 × 10−7 | 0.76 | 1.34 | 0.50 | 56.42% | OFF |
Notes. Column (1) means run name. Column (2) presents the density at the center of the initial torus. Column (3) gives the net accretion rate at inner boundary. Column (4) gives the power-law indices for the inflow, characterized by a radial profile proportional to rsin. Column (5) gives the power-law indices for the outflow, characterized by a radial profile proportional to rsout. Column (6) gives the Power-law indices for the density at the equational panel. The density is described by a radial profile that is proportional to r−p. Column (7) gives the proportion of the area occupied by the convectively stable regions within the accretion disk. Column (8) means that radiative cooling was either included or excluded. “ON” means that radiative cooling was implemented during the simulation, while “OFF” indicates that it was not.
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.