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Table 3
The predicted number of massive stars of each model.
| Nmassive outside the clusters | |||||||
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| WR-L = 20 M⊙ | StdDev | WR-L = 40 M⊙ | StdDev | WR-L = 60 M⊙ | StdDev | ||
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| Qage = 4 Myr | 62 | σ4,20 = 8 | 22 | σ4,40 = 5 | 11 | σ4,60 = 4 | |
| Qage = 4.5 Myr | 80 | σ4.5,20 = 12 | 30 | σ4.5,40 = 4 | 13 | σ4.5,60 = 2 | |
| Qage = 5.0 Myr | 68 | σ5,20 = 8 | 26 | σ5,40 = 3 | 10 | σ5,60 = 2 | |
Notes. In the Pa survey region, 35 massive stars are observed outside the three clusters (outside their approximate tidal radius) in the GC region. Among these massive stars are 24 Wolf-Rayet stars.
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