Table 7
SPEFO RVs of the wings and two line cores of the He i 5876 Å line and RVs from Gaussian fits of the He ii 5411 Å line of HD 123056 (in km s-1).
| RJD | 5876 | O−C | 5876 | 5876 | 5411 | O−C | Spectro- |
| wings | core | 2nd core | graph | ||||
|
|
|||||||
| 34 825.5256 | −30.00 | −5.0 | R | ||||
| 34 834.4991 | −23.00 | 3.3 | R | ||||
| 35 181.5451 | −59.00 | −8.3 | R | ||||
| 35 208.4685 | −44.00 | 5.0 | R | ||||
| 54 935.6907 | −38.23 | 9.7 | −2.10 | – | −36 | 9.8 | B |
| 54 952.7769 | −53.41 | −6.8 | −3.59 | – | −48 | −3.3 | B |
| 54 954.7400 | −52.74 | −6.2 | 19.43 | −88.48 | −53 | −8.4 | F |
| 54 960.7492 | −48.83 | −2.8 | −47.60 | – | −51 | −6.8 | B |
| 54 976.6593 | −39.31 | 5.5 | −49.72 | – | −38 | 5.1 | F |
| 55 240.9051 | −10.76 | 12.1 | 28.73 | −68.46 | −12 | 10.9 | B |
| 55 241.9183 | −18.94 | 3.8 | 14.42 | – | −23 | −0.2 | B |
| 55 251.8066 | −19.02 | 3.0 | −31.34 | – | −22 | 0.1 | B |
| 55 253.8783 | −35.55 | −13.7 | 19.24 | −96.36 | −28 | −6.1 | B |
| 55 605.8938 | −11.34 | −4.6 | 7.84 | −89.40 | −13 | −7.8 | F |
| 55 642.7878 | −14.63 | −7.3 | −3.83 | – | −11 | −5.2 | F |
| 55 697.7150 | −1.42 | 8.0 | −60.12 | 22.53 | −2 | 6.2 | F |
| 55 698.7538 | −5.48 | 4.0 | −4.33 | – | −5 | 3.2 | F |
| 55 794.9821 | −16.54 | 1.0 | 3.44 | – | −15 | 2.8 | B |
| 55 803.9761 | −13.59 | 5.0 | −37.69 | – | −16 | 3.1 | B |
| 55 805.9746 | −12.87 | 6.0 | 7.33 | – | −7 | 12.3 | B |
| 56 067.7858 | −48.14 | 4.2 | −57.94 | – | −45 | 5.5 | F |
| 56 068.7840 | −52.54 | −0.1 | −4.48 | – | −53 | −2.5 | F |
| 57 155.8197 | −24.22 | −0.6 | −41.14 | 29.73 | −33 | −8.3 | F |
| 57 156.8305 | −27.45 | −3.7 | −38.31 | – | −28 | −3.2 | F |
| 57 157.7282 | −19.56 | 4.4 | 24.60 | −88.29 | −27 | −2.0 | F |
| 57 159.7152 | −26.52 | −2.3 | 18.48 | – | −26 | −0.7 | F |
| 57 160.5437 | −33.10 | −8.8 | −56.91 | – | −30 | −4.6 | F |
Notes. The four early Radcliffe RVs (R) are the mean RVs of several spectral lines. To estimate the measurement errors of the components of He i 5876 Å in SPEFO, we repeated the measurements several times independently. The results for the wings usually differed by less than 1 km s-1, while the settings for the line cores are less certain, especially for lower S/N BESO spectra.
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