Table 1
Initial conditions for the stellar models.
| Model | MZAMS,l | MZAMS | q | P | e | N (×107) |
|---|---|---|---|---|---|---|
| kro1 | Kroupa (2001) | Flat in log | S12 | S12 | S12 | 2 |
| kro5 | Kroupa (2001) | Flat in log | SB13 | SB13 | Thermal | 2 |
| lar1 | Larson (1998) | – | S12 | S12 | S12 | 2 |
| lar5 | Larson (1998) | – | SB13 | SB13 | Thermal | 2 |
| log1 | Flat in log | – | S12 | S12 | S12 | 1.45 |
| log2 | Flat in log | – | S12 | SB13 | Thermal | 1.45 |
| log3 | – | – | Sorted | S12 | S12 | 1.38 |
| log4 | – | – | SB13 | S12 | Thermal | 1.53 |
| log5 | Flat in log | – | SB13 | SB13 | Thermal | 1.53 |
| top1 | Top heavy | – | S12 | S12 | S12 | 1.05 |
| top5 | Top heavy | Flat in log | SB13 | SB13 | Thermal | 1.07 |
Notes. Column 1: model name. Column 2: IMF for the primary star. Column 3: ZAMS mass of the whole stellar population. Columns 4, 5, and 6: initial distributions for the mass ratio q, period P, and eccentricity e. The acronyms S12 and SB13 refer to Sana et al. (2012) and Stacy & Bromm (2013), respectively. Column 7: total number of simulated stars.
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