Table 1
Initial cluster model adopted by Portegies Zwart (2016); the final conditions for the disk-size analysis in Portegies Zwart (2016), which we adopted as the initial realization for the simulations presented here; and the final conditions.
| Parameter | t = 0 Myr | t = 1 Myr | t = 11 Myr |
|---|---|---|---|
| Cluster characteristics | |||
| Ntotal | 1500 | 1500 | 1482 |
| Mbnd/M⊙ | 627 | 618 | 545 |
| Rvir/pc | 0.5 | 0.36 | 0.32 |
| Q | 1.0 | 0.6 | 1.0 |
| F | 1.6 | 1.26 | 0.6 |
| Stellar characteristics | |||
| Nbnd | 1500 | 977 | 508 |
| Nbnd,w/p | 0 | 512 | 166 |
| Nunbnd,w/p | 0 | 0 | 323 |
| Nw/planets | 0 | 500 | 517 |
| Nr≥100 au | 1500 | 78 | |
| Nr≥10 au | 1500 | 578 | |
| Planets characteristics | |||
| nbnd | – | 2522 | 2165 |
| nff | – | 0 | 357 |
| nunbnd | – | 0 | 282 |
| mbnd/MJup | – | 3527 | 2915 |
| mff/MJup | – | 0 | 502 |
| munbnd/MJup | – | 0 | 395 |
Notes. The parameter Ntotal indicates the total number of stars in the simulation; Nbnd, the bound mass of the cluster in solar masses; Rvir the virial radius of the cluster; Q, the virial equilibrium; F, the fractal dimension of the cluster; Nbnd, the number of bound stars;Nbnd, the number of bound stars with planets; Nbnd, the number of unbound stars with planets; Nw/planets, the number of stars with planets; Nr≥100 au the number of stars with disks or planets equal or larger than 100 au; Nr≥100 au the number of stars with disks or planets equal or larger than 10 au; nbnd, the number of planets bound to a star; nff, the number of free-floating planets; nunbnd, the number of planets unbound from the cluster; mbnd, the total planetary mass in Jupiter masses, bound to a star; mff, the total planetary mass in free-floating planets; and munbnd, the total planetary mass unbound from the cluster.
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