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Table 3.
MWDs in binary star systems.
| Villanova | Spectral | Mass | V | Dist | ⟨|B|⟩ | ⟨Bz⟩ | System | MS | Proj sep | References |
|---|---|---|---|---|---|---|---|---|---|---|
| WD name | class | (M⊙) | (mag) | (pc) | (MG) | (MG) | type | star | (AU) | |
| 0301+059 | DA(?)P | 1.1 | 15 | 31.4 | 200? | Sirius-like | G0V | 377 | This work | |
| 1009−184 | DZH8.5 | 0.53 | 15.44 | 18.1 | <0.3 | 0.05 | Sirius-like | K7 | 7240 | H13, H16, T17, B19 |
| 1105−048 | DAH3.5 | 0.60 | 12.92 | 24.8 | <0.02 | 0.003 | WD+dM | M3 | 6920 | A04, H16, T17, B18 |
| 2154−512 | DQH8.3 | 0.60 | 14.74 | 14.9 | >4 | 1.3 | WD+dM | M2 | 417 | V10, H16, T17 |
| NGC 2422 | DBH | 1.06 | 19.8 (G) | 500 | 2.5 | WD+dM | dM: | <250 | R19 |
Notes. Key to references: A04: Aznar Cuadrado et al. (2004); V10: Vornanen et al. (2010); H13: Holberg et al. (2013); H16: Holberg et al. (2016); T17: Toonen et al. (2017); B18: Bagnulo & Landstreet (2018); B19: Bagnulo & Landstreet (2019b); R19: Richer et al. (2019).
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