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Table 3
Known DZ and DZA WDs within 20 pc from the Sun for which we need more highly-sensitive spectropolarimetric measurements.
| d | Teff | Age | |||||||
|---|---|---|---|---|---|---|---|---|---|
| STAR | V | (pc) | Spectrum | (K) | log g | M∕M⊙ | (Gyr) | log(L∕L⊙) | References |
| WD 0046+051 | 12.4 | 4.32 | DZ8.2 | 6130 | 8.16 | 0.67 | 3.45 | −3.79 | 1,3 |
| WD 0552–041 | 14.5 | 6.44 | DZ9.3 | 5430 | 8.49 | 0.90 | 7.34 | −4.20 | 1,3 |
| WD 0738–172 | 13.1 | 9.16 | DZ6.5 | 7700 | 8.05 | 0.61 | 1.31 | −3.33 | 1,3 |
| WD 0840–136 | 15.7 | 14.80 | DZ10.1 | 4980 | 7.95 | 0.54 | 5.28 | −4.04 | 1,3 |
| WD 1626+368 | 14.0 | 15.89 | DZA5.9 | 8507 | 8.00 | 0.58 | 1.02 | −3.13 | 2,3 |
| WD 1705+030 | 15.2 | 17.87 | DZ7.7 | 6584 | 8.18 | 0.68 | 2.75 | −3.67 | 2,3 |
| WD 2251–070 | 15.7 | 8.53 | DZ12.6 | 4000 | 7.92 | 0.52 | 7.13 | −4.40 | 1,3 |
Notes. Key to references is given in Table 1.
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