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|
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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