Table 7.
WD masses derived from the astrometrically based sin i (Pourbaix & Jorissen 2000) and from the assumption of constant Q.
| HD | HIP | Ba | MBa | f(M) | i | MWD |
|
|---|---|---|---|---|---|---|---|
| (i) | (Q) | ||||||
| (M⊙) | (M⊙) | (°) | (M⊙) | (M⊙) | |||
| 46407 | 31205 | s | 2.12 | 0.035 | 80 ± 10 | 0.71 |
0.78 |
| 101013 | 56731 | s | 1.65 | 0.037 | 78 ± 26 | 0.59 |
0.68 |
Notes. The error bars for the WD mass derived from astrometry correspond to the error propagation from the inclination. The column labeled “Ba” lists whether the star is a mild (“m”) or strong (“s”) barium star.
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