Table 2.
Programme stars and their main physical features.
Star | G | d | Teff | log g | M | Age | Atmosphere and ref. | |
---|---|---|---|---|---|---|---|---|
(pc) | (K) | c.g.s. | (M⊙) | (Gyr) | ||||
WD 0005+395 | LP 240-30 | 16.6 | 34.4 | 4680 | 6.77 | 0.08 | 1.40 | DC, H ProbWD = 0.70 (1,3) |
WD 0010+543 | LSR J0013+5437 | 18.0 | 32.3 | 4123 | 7.77 | 0.46 | 7.08 | DC, (2, H assumed) |
WD 0028+035 | PB 6002 | 16.1 | 27.8 | 6548 | 8.14 | 0.68 | 2.40 | DC, (2, H assumed) |
WD 1251+366 | LP 267-311 | 17.2 | 28.5 | 4445 | 7.62 | 0.37 | 3.78 | DC, He (1) |
WD 1315+222 | LP 378-956 | 16.7 | 31.8 | 6235 | 8.21 | 0.71 | 3.61 | DCH, He (1) |
WD 1346+121 | LP 498-66 | 17.8 | 28.3 | 4150 | 7.88 | 0.50 | 6.58 | DCH, He (1) |
WD 1425+495 | CSO 649 | 16.7 | 33.9 | 6895 | 8.41 | 0.85 | 3.77 | DC, (2, H assumed) |
WD 1427−238 | LP 857-45 | 17.4 | 32.6 | 4866 | 7.90 | 0.52 | 5.40 | DC, (2, H assumed) |
WD 1434+437 | LP 221-217 | 17.2 | 27.2 | 4685 | 7.93 | 0.54 | 6.30 | DC, H–He (1) |
WD 1533+469 | LP 176-60 | 17.8 | 30.8 | 4310 | 7.83 | 0.48 | 6.45 | DC?, H (1) |
WD 1601-073 | LP 684-16 | 17.9 | 26.9 | 4920 | 8.55 | 0.94 | 9.83 | DCH, (2, H assumed) |
WD 1612+092 | LSPM J1614+0906 | 17.2 | 27.9 | 4775 | 7.90 | 0.52 | 5.57 | DC, H (1) |
WD 1702−016 | LP 626-29 | 17.3 | 28.3 | 4700 | 7.94 | 0.54 | 6.50 | DC, (2, H assumed) |
WD 1737+798 | LP 24-66 | 16.9 | 26.8 | 5535 | 8.28 | 0.75 | 5.72 | DC, He (1) |
WD 1746+450 | GD 366 | 15.5 | 29.9 | 9331 | 8.47 | 0.90 | 1.72 | DC, (2, H assumed) |
WD 1800+508 | LP 139-38 | 17.4 | 31.0 | 4635 | 7.85 | 0.48 | 5.12 | DC, He–H (1) |
WD 1853+775 | LP 25-7 | 17.0 | 30.5 | 4850 | 7.74 | 0.43 | 3.63 | DCH, He (1) |
WD 2058+550 | LSR J2059+5517 | 17.1 | 22.7 | 4415 | 7.93 | 0.53 | 7.15 | DC, H–He (1) |
WD 2109−295 | EC 21096-2934 | 15.1 | 32.8 | 9260 | 7.98 | 0.57 | 0.78 | DC, He–H (3) |
WD 2152−280 | LP930-61 | 16.3 | 23.5 | 5220 | 7.85 | 0.48 | 3.68 | DC, He (1) |
WD 2211+372 | LP 287-35 | 16.8 | 29.2 | 6345 | 8.47 | 0.88 | 4.56 | DC?H, He (1) |
WD 2215+368 | LP 287-39 | 16.8 | 20.3 | 4485 | 7.92 | 0.53 | 6.80 | DC, H (1) |
WD 2311−068 | G 157-34 | 15.3 | 25.9 | 7360 | 7.97 | 0.56 | 1.31 | DC, He (1) |
Notes. Star names in boldface identify WDs in which fields were discovered during the observations reported in this paper (see Table 3). References. 1: Blouin et al. (2019); 2: Gentile Fusillo et al. (2021); 3: Bergeron et al. (2021). Where not found in these references, ages have been interpolated using the tables from Bédard et al. (2020).
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