Table 1
Initial conditions for the stellar models.
| Model | mZAMS,1 | mZAMS | q | P | e |
|---|---|---|---|---|---|
| kro1 | Kroupa (2001) | Flat in log | S12 | S12 | S12 |
| kro5 | Kroupa (2001) | Flat in log | SB13 | SB13 | Thermal |
| lar1 | Larson (1998) | − | S12 | S12 | S12 |
| lar5 | Larson (1998) | − | SB13 | SB13 | Thermal |
| log1 | Flat in log | – | S12 | S12 | S12 |
| log2 | Flat in log | − | S12 | SB13 | Thermal |
| log3 | − | − | Sorted | S12 | S12 |
| log4 | – | – | SB13 | S12 | Thermal |
| log5 | Flat in log | − | SB13 | SB13 | Thermal |
| top1 | Top heavy | − | S12 | S12 | S12 |
| top5 | Top heavy | Flat in log | SB13 | SB13 | Thermal |
Notes. Column 1: name of the model. Column 2: IMF of the primary star. Column 3: ZAMS mass of the overall stellar population. Columns 4-6: 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.
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