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Table 4
Stripped mass.
| Model | Mc,f | af/R2 | ΔM1 | ΔM2 | Difference |
| [M⊙] | [M⊙] | [M⊙] | [%] | ||
|
|
|||||
| ms_20a | 0.74 | 3.06 | 0.18 | 0.19 | 5 |
| ms_20b | 1.17 | 2.75 | 0.11 | 0.14 | 27 |
| ms_22a | 1.21 | 2.72 | 0.17 | 0.18 | 6 |
| ms_20c | 1.22 | 2.71 | 0.17 | 0.14 | 18 |
| ms_24a | 1.40 | 2.63 | 0.17 | 0.19 | 12 |
| ms_20d | 1.40 | 2.63 | 0.11 | 0.15 | 36 |
| ms_23a | 1.50 | 2.59 | 0.16 | 0.19 | 19 |
| ms_24b | 1.88 | 2.46 | 0.12 | 0.17 | 42 |
| ms_28a | 2.00 | 2.43 | 0.16 | 0.21 | 32 |
| ms_30a | 2.45 | 2.33 | 0.14 | 0.20 | 43 |
Notes.
(2)
Stripped mass analytically estimated by using the method of Wheeler et al. (1975). Here, we directly use the density profiles of companion models from the 1D stellar evolution calculations.
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