Table 1.
Initial conditions involved in this study.
Mcl [M⊙] | Rcl [pc] | tff [Myr] | mgas [M⊙] |
![]() |
![]() |
ϵw, c | vw, c [km/s] | NBH |
![]() |
Notes |
---|---|---|---|---|---|---|---|---|---|---|
106 | 5 | 0.19 | 3.8 | 0.41 | 0.31 | 10−6 | 420 | 234 | 10–103 | Low res. |
106 | 5 | 0.19 | 0.48 | 0.21 | 0.21 | 10−6 | 420 | 234 | 10–103 | High res. |
108 | 50 | 0.59 | 380 | 1.9 | 0.31 | 10−3 | 13 000 | 2000 | 102–104 | Low res. |
108 | 50 | 0.59 | 48 | 0.96 | 0.31 | 10−3 | 13 000 | 2000 | 102–104 | High res. |
Notes. We chose some gas complexes in the “high-surface-density” (Σ0 = 13000 M⊙ pc−2) group of Paper I, with an initial radius (Rcl) of 5 pc or 50 pc. Each kind of gas complex is simulated at high and low resolution. Starting from the third column, we show the initial free-fall time (tff), gas mass resolution (mgas), softening radius for stars () and BHs (
), characteristic jet energy efficiency (ϵw, c), and velocity (vw, c) as described in Sect. 2, as well as the number of BH seeds (NBH), and the initial BH mass (
) for different kinds of simulations.
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.