Table 2.
Spectroscopic binaries with no orbits yet available (flagged in bold face and as “SB” in the last column) and objects with no variability detected.
| std(RV) | 3σ(RV) | ||
|---|---|---|---|
| Name | [km s−1] | [km s−1] | Comments |
| BD–11°3853 | 2.37 | 0.37 | SB |
| CD–62°1346 | 2.03 | 1.70 | SB |
| HD 2454(1) | 0.5863 | 0.1917 | SB |
| HD 6434 | 0.44 | 0.95 | |
| HD 9529 | 0.59 | 1.52 | |
| HD 13555(2) | 0.14 | 0.33 | |
| HD 18853 | 2.43 | 1.03 | SB |
| HD 26455 | 5.15 | 1.63 | SB2 |
| HD 31732 | 0.30 | 1.23 | |
| HD 35296 | 0.24 | 0.59 | |
| HD 60532 | 0.15 | 0.31 | |
| HD 69578 | 17.99 | 1.65 | SB |
| HD 82328 | 0.13 | 0.25 | |
| HD 92545 | 0.50 | 0.42 | SB |
| HD 101581 | 0.10 | 0.88 | |
| HD 103840 | 0.52 | 0.97 | |
| HD 104342 | 0.58 | 1.17 | |
| HD 105671 | 0.31 | 0.94 | |
| HD 109490 | 14.67 | 7.54 | SB |
| HD 113402 | 1.06 | 2.91 | |
| HD 117288 | 0.50 | 1.08 | |
| HD 124850 | 0.42 | 0.51 | |
| HD 130255 | 0.21 | 0.43 | |
| HD 146800 | 0.21 | 0.99 | |
| HD 170149 | 0.42 | 1.47 | |
| HD 177996 | 9.53 | 1.18 | SB2 |
| HD 188985 | 1.03 | 0.69 | SB |
| HD 202400 | 4.03 | 4.21 | |
| HD 205156 | 1.40 | 1.18 | SB |
| HD 219899 | 0.36 | 0.96 | |
| HD 220117 | 0.17 | 0.47 | |
| HD 222349 | 3.26 | 1.35 | SB |
| HD 224621 | 6.32 | 0.98 | SB |
Notes. The second column (std(RV)) gives the standard deviation of the RV points and the third column (3σ(RV)) gives three times the average error bar considering all the RV points. We claim that a star is in a binary system when the number in the second column is higher than that in the third column.
(1)std(RV) and 3σ(RV) were computed using only HERMES data. Binarity is clear from this data set, while the CORAVEL RV points are very scattered (see third panel of Fig. B.26).
(2)std(RV) and 3σ(RV) were computed excluding the second CORAVEL RV point, which we considered an outlier (see third panel of Fig. B.27).
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