Physical parameters characterizing our initial cluster models. The values of r0 and τg are strictly related, while those of τd are independent.
| Parameter . | Notation . | Values . |
|---|---|---|
| Number of stars | N | 1000 |
| Star formation efficiency | ϵ | 0.33 |
| Plummer radius (pc) | r0 | 0.585, 1.17 |
| Gas expulsion delay (Myr) | τd | 0.6, 2.4 |
| Gas expulsion e-folding time (Myr) | τg | 0.077, 0.153 |
| Virial ratio (target) | Q | 0.15 |
| Binary fraction | fbin | 0.3 |
| Mass segregation strength | s | 0.5 |
| Parameter . | Notation . | Values . |
|---|---|---|
| Number of stars | N | 1000 |
| Star formation efficiency | ϵ | 0.33 |
| Plummer radius (pc) | r0 | 0.585, 1.17 |
| Gas expulsion delay (Myr) | τd | 0.6, 2.4 |
| Gas expulsion e-folding time (Myr) | τg | 0.077, 0.153 |
| Virial ratio (target) | Q | 0.15 |
| Binary fraction | fbin | 0.3 |
| Mass segregation strength | s | 0.5 |
Physical parameters characterizing our initial cluster models. The values of r0 and τg are strictly related, while those of τd are independent.
| Parameter . | Notation . | Values . |
|---|---|---|
| Number of stars | N | 1000 |
| Star formation efficiency | ϵ | 0.33 |
| Plummer radius (pc) | r0 | 0.585, 1.17 |
| Gas expulsion delay (Myr) | τd | 0.6, 2.4 |
| Gas expulsion e-folding time (Myr) | τg | 0.077, 0.153 |
| Virial ratio (target) | Q | 0.15 |
| Binary fraction | fbin | 0.3 |
| Mass segregation strength | s | 0.5 |
| Parameter . | Notation . | Values . |
|---|---|---|
| Number of stars | N | 1000 |
| Star formation efficiency | ϵ | 0.33 |
| Plummer radius (pc) | r0 | 0.585, 1.17 |
| Gas expulsion delay (Myr) | τd | 0.6, 2.4 |
| Gas expulsion e-folding time (Myr) | τg | 0.077, 0.153 |
| Virial ratio (target) | Q | 0.15 |
| Binary fraction | fbin | 0.3 |
| Mass segregation strength | s | 0.5 |
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