Table G.1.
Overview of binary evolution models computed with MESA.
| Md, initial | Ma, initial | Pinitial | β | Md, stripped | Ma, Be | P | |
|---|---|---|---|---|---|---|---|
| M1 | 4.0 M⊙ | 3.6 M⊙ | 12 d | 0.0 | 0.72 M⊙ | 6.9 M⊙ | 277 d |
| M2 | 5.0 M⊙ | 4.5 M⊙ | 8 d | 0.7 | 0.88 M⊙ | 5.7 M⊙ | 263 d |
| M3 | 5.5 M⊙ | 5.0 M⊙ | 8 d | 0.7 | 0.99 M⊙ | 6.3 M⊙ | 247 d |
| M4 | 6.0 M⊙ | 5.4 M⊙ | 8 d | 0.7 | 1.12 M⊙ | 6.8 M⊙ | 230 d |
| M5 | 7.0 M⊙ | 4.2 M⊙ | 8 d | 0.7 | 1.37 M⊙ | 8.0 M⊙ | 197 d |
| M3a | 5.5 M⊙ | 2.8 M⊙ | 30 d | 0.0 | 1.00 M⊙ | 7.3 M⊙ | 275 d |
| M3b | 5.5 M⊙ | 3.9 M⊙ | 12 d | 0.5 | 0.99 M⊙ | 6.1 M⊙ | 224 d |
| M3c | 5.5 M⊙ | 5.0 M⊙ | 8 d | 0.7 | 0.99 M⊙ | 6.3 M⊙ | 247 d |
| M3d | 5.5 M⊙ | 5.2 M⊙ | 5 d | 0.9 | 0.97 M⊙ | 5.6 M⊙ | 189 d |
Notes. Columns list the model index, initial stellar masses and periods, mass accretion efficiency, masses and periods during the stripped star phase. The first set of models is computed with varying primary star masses. For the second set of models with indices 3a - 3d, Md, initial is fixed to 5.5 M⊙.
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