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Table 2.
Parameters of MS−BD binaries inferred from WD−BD binaries using a population synthesis technique.
| System | MMS | Initial Period | Periodpre − CE | αCE |
|---|---|---|---|---|
| /M⊙ | /day | /day | ||
| SDSS J1411+2009 | 1.02 − 1.44 | 336 − 583 | 387 − 978 | 0.12 − 0.41 |
| SDSS J1205−0242 | 1.00 − 1.48 | 72 − 178 | 74 − 219 | 0.14 − 0.90 |
| WD 1032+011 | 1.00 − 1.24 | 137 − 430 | 150 − 721 | 0.09 − 0.45 |
| ZTF J0038+2030 | 1.00 − 1.10 | 402 − 486 | 738 − 1004 | 0.45 − 0.95 |
| WD 0137−349 | 1.00 − 1.56 | 65 − 213 | 68 − 270 | 0.16 − 1.00 |
| NLTT 5306 | 1.00 − 1.22 | 136 − 407 | 149 − 663 | 0.10 − 0.45 |
| SDSS J1557+0916 | 1.00 − 1.72 | 123 − 409 | 127 − 667 | 0.09 − 1.00 |
| EPIC 212235321 | 1.08 − 1.56 | 264 − 389 | 280 − 568 | 0.09 − 0.49 |
Notes. The initial period refers to the orbital period when the primary star starts its MS evolution. In our calculation, we have added minimum total age constraints on these systems.
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