Table 1
Sample of binary systems with a WD companion and known orbital elements.
Names | Spectral type | MWD (M⊙) | P (d) | e | f(M1,M2) (M⊙) | Ref. |
|
||||||
EUVE J0459-102 | G4V + He WD | 0.3 | 903 ± 5 | 0.30 ± 0.06 | 0.009 ± 0.003 | 2, 3 |
HR 1608 (63 Eri) | ||||||
HD 185510 (V1379 Aql) | K0III + sdB | 0.30−0.36 | 20.66187 ± 0.00058 | 0.094 ± 0.011 | 0.0042 ± 0.0002 | 1 |
EUVE J0254-053 | K0 IV + He WD | 0.4 | 1071.0 ± 1.8 | 0.25 ± 0.01 | 0.0036 ± 0.0001 | 4, 5 |
HD 18131 (IP Eri) | ||||||
EUVE J0515+326 | F3V | 0.53−0.69 | 2.99322 ± 0.00005 | 0 | 0.0079 ± 0.0002 | 3 |
HD 33959C (14 Aur C) | ||||||
EUVE J1732+74.2 | K0III | 0.55 | 903.8 ± 0.4 | 0.07 ± 0.03 | 0.0035 ± 0.0003 | 1, 17 |
HD 160538 (DR Dra) | ||||||
HD 35155 (V1261 Ori) | S4,1 | 0.55 ± 0.05 | 640.7 ± 2.7 | 0.07 ± 0.03 | 0.032 ± 0.003 | 6, 7 |
1RXS J151824.6+203423 | G8III Ba0.3 | 0.59−0.79 | 506.45 ± 0.18 | 0.3353 ± 0.0056 | 0.0112 ± 0.0003 | 6, 8 |
HR 5692 | ||||||
HD 121447 (IT Vir) | K7III Ba SC2 | 0.5−0.7 | 185.66 ± 0.07 | 0.0 | 0.025 ± 0.001 | 16 |
HD 202109 (ζ Cyg) | G8III Ba0.6 | 0.7−1.1 | 6489 ± 31 | 0.22 ± 0.03 | 0.023 ± 0.003 | 9, 10, 14 |
RX J2307.1+2528 | K0Iab Ba | 0.75−1.15 | 111.14 ± 0.01 | 0 | (3.7 ± 0.3)10-5 | 11, 12, 13 |
HR 8796 (56 Peg) | ||||||
ζ Cap | G4Ib Ba | 1 | 2378 ± 55 | 0.28 ± 0.07 | 0.004 ± 0.001 | 14, 15 |
HD 204075 |
Notes. P and e are the orbital period and eccentricity and f(M1,M2) is the mass function, ordered by increasing WD mass.
Reference. (1) Fekel et al. (1993); (2) Landsman et al. (1993); (3) Vennes et al. (1998) (4) Burleigh et al. (1997); (5) Merle et al. (2014); (6) Jorissen et al. (1996); (7) Jorissen et al. (1992); (8) Stefanik et al. (2011); (9) Dominy & Lambert (1983); (10) Griffin & Keenan (1992); (11) Schindler et al. (1982); (12) Griffin (2006); (13) Frankowski & Jorissen (2006); (14) Böhm-Vitense (1980); (15) Jorissen et al. (1998); (16) Jorissen et al. (1995); (17) Fekel & Simon (1985).
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