Table 1.
Types of objects that originated from different types of stellar mergers based on Table 2 from Hurley et al. (2002).
| First stellar type k1 | ||||||||||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 0 | 1 | 2 | 3 | 4 | 5 | 6 | 7 | 8 | 9 | 10 | 11 | 12 | 13 | 14 | ||
| 0 | 1 | 1 | 2 | 3 | 4 | 5 | 6 | 4 | 6 | 6 | 3 | 6 | 6 | 13 | 14 | |
| 1 | 1 | 1 | 2 | 3 | 4 | 5 | 6 | 4 | 6 | 6 | 3 | 6 | 6 | 13 | 14 | |
| 2 | 2 | 2 | 3 | 3 | 4 | 4 | 5 | 4 | 4 | 4 | 3 | 5 | 5 | 13 | 14 | |
| 3 | 3 | 3 | 3 | 3 | 4 | 4 | 5 | 4 | 4 | 4 | 3 | 5 | 5 | 13 | 14 | |
| 4 | 4 | 4 | 4 | 4 | 4 | 4 | 4 | 4 | 4 | 4 | 4 | 4 | 4 | 13 | 14 | |
| Second | 5 | 5 | 5 | 4 | 4 | 4 | 4 | 4 | 4 | 4 | 4 | 4 | 4 | 4 | 13 | 14 |
| stellar | 6 | 6 | 6 | 5 | 5 | 4 | 4 | 6 | 4 | 6 | 6 | 5 | 6 | 6 | 13 | 14 |
| type | 7 | 4 | 4 | 4 | 4 | 4 | 4 | 4 | 7 | 8 | 9 | 7 | 9 | 9 | 13 | 14 |
| k2 | 8 | 6 | 6 | 4 | 4 | 4 | 4 | 6 | 8 | 8 | 9 | 7 | 9 | 9 | 13 | 14 |
| 9 | 6 | 6 | 4 | 4 | 4 | 4 | 6 | 9 | 9 | 9 | 7 | 9 | 9 | 13 | 14 | |
| 10 | 3 | 3 | 3 | 3 | 4 | 4 | 5 | 7 | 7 | 7 | 15 | 9 | 9 | 13 | 14 | |
| 11 | 6 | 6 | 5 | 5 | 4 | 4 | 6 | 9 | 9 | 9 | 9 | 11 | 12 | 13 | 14 | |
| 12 | 6 | 6 | 5 | 5 | 4 | 4 | 6 | 9 | 9 | 9 | 9 | 12 | 12 | 13 | 14 | |
| 13 | 13 | 13 | 13 | 13 | 13 | 13 | 13 | 13 | 13 | 13 | 13 | 13 | 13 | 13 | 14 | |
| 14 | 14 | 14 | 14 | 14 | 14 | 14 | 14 | 14 | 14 | 14 | 14 | 14 | 14 | 14 | 14 | |
Notes. The numeric types are consistent with Hurley et al. (2002): 0 – main sequence star with M < =0.7 M⊙ (deeply or fully convective); 1 – main sequence star with M > 0.7 M⊙; 2 – Hertzsprung gap star; 3 – first giant branch star; 4 – core helium burning star; 5 – early asymptotic giant branch star; 6 – thermally pulsing asymptotic giant branch star; 7 – main sequence naked helium star; 8 – Hertzsprung gap naked helium star; 9 – giant branch naked helium star; 10 – helium white dwarf; 11 – carbon or oxygen white dwarf; 12 – oxygen or neon white dwarf; 13 – neutron star; 14 – black hole; 15 – massless remnant.
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