Table A.1
Masses of different stellar components.
| Salpeter | Kroupa | Miller-Scalo | |
|
|
|||
| m MS | 0.21 M⊙ | 0.28 M⊙ | 0.29 M⊙ |
| m WD | 0.78 M⊙ | 0.79 M⊙ | 0.77 M⊙ |
| m NS | 1.59 M⊙ | 1.59 M⊙ | 1.57 M⊙ |
| m BH | 6.80 M⊙ | 6.59 M⊙ | 6.59 M⊙ |
| m DR | 0.85 M⊙ | 0.81 M⊙ | 0.79 M⊙ |
| m MS / m DR | 0.24 | 0.35 | 0.37 |
| M MS / M DR | 3.88 | 2.10 | 1.47 |
Notes. Mean values for the masses of the typical main-sequence star (MS), white dwarf (WD), neutron star (NS), and black hole (BH). By dark remnant (DR) we mean all the possible remnants in the cluster. The last row represents the ratio of the total masses.
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