Table 1
Parameters of Eqs. (2) and (3).
| N | B | C | D | E |
|---|---|---|---|---|
| 100 | 0.45 ± 0.02 | − 2.25 ± 0.06 | 0.40 ± 0.04 | − 0.16 ± 0.09 |
| 500 | 0.49 ± 0.02 | −2.27 ± 0.06 | 0.53 ± 0.04 | 0.22 ± 0.09 |
| 1000 | 0.51 ± 0.04 | −2.29 ± 0.09 | 0.57 ± 0.06 | 0.44 ± 0.14 |
| 5000 | 0.50 ± 0.03 | −2.16 ± 0.07 | 0.52 ± 0.05 | 1.28 ± 0.12 |
Notes. Parameters from the fit to Eqs. (2) (Cols. 2 and 3) and (3) (Cols. 4 and 5) to estimate the total fraction of collisions in a cluster depending on the initial radii of the stars Rstar and the initial number N of stars (Eq. (2)). Parameters D and E are used to estimate the mass of the most massive object divided by its initial mass (Mmax ∕Mini) at the end of the runaway growth, depending on the initial radii Rstar of the stars and the initial number N of stars (Eq. (3)).
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