Table 1
N-body simulations of subcluster coalescence and cluster evolution under different gas expulsion modes.
| Cases | Type | Mass (M⊙) | Time (Myr) | Dissolved(hr/) |
|---|---|---|---|---|
| 10 000-fast | Individual | 10 000 | 263 | Yes |
| 3000-fast | Individual | 3000 | 100 | Yes |
| 3000-moderate1 | Individual | 3000 | 441 | No |
| 3000-moderate2 | Individual | 3000 | 256.25 | Yes |
| 3000-slow | Individual | 3000 | 950.25 | Yes |
| 1000-fast | Individual | 1000 | 67.5 | Yes |
| 1000-moderate1 | Individual | 1000 | 145.5 | Yes |
| 1000-moderate2 | Individual | 1000 | 78 | Yes |
| 1000-slow | Individual | 1000 | 533.5 | Yes |
| 300-fast | Individual | 300 | 69 | Yes |
| 300-moderate1 | Individual | 300 | 100 | Yes |
| 300-moderate2 | Individual | 300 | 45.25 | Yes |
| 300-slow | Individual | 300 | 346.5 | Yes |
| NGC6334-fast | Coalescence | 2207 | 614.25 | Yes |
| NGC6334-fast-vd | Coalescence | 2207 | 463.75 | Yes |
Notes. The table lists N-body simulations modeling both the coalescence of multiple subclusters and the evolution of individual clusters under different gas-expulsion modes. More details are provided in Sect. 2 and Appendix A. “Time” denotes the point at which the simulation is terminated; the cluster may or may not have dissolved by this time.
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