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Table 1

Best-fit orbital parameters of HD 152218.

Parameter Stickland et al. (1997) Sana et al. (2008a) This work

New FEROS RVs All RV data Echelle spectra
[ 1] [ 2] [ 3] [ 4] [ 5]

Porb (d) 5.603979 5.60391 5.60400 ± 0.00004
e 0.308 ± 0.018 0.259 ± 0.006 0.269 ± 0.005
ω (°) 80.6 ± 2.1 104.0 ± 1.6 103.4 ± 0.9
(° yr-1) 1.43.2
ω0 (°)
T0 (HJD2 400 000) 48 865.024 ± 0.028 53 197.229 ± 0.025 53 129.986 ± 0.015
q = m1/m2 1.341 ± 0.030 1.319 ± 0.014 1.320 ± 0.011
K1 (km s-1) 156.9 ± 3.6 162.2 ± 1.2 160.3 ± 1.0
K2 (km s-1) 210.4 ± 3.5 213.9 ± 1.5 211.5 ± 1.3
γ1 (km s-1) −26.6 ± 1.9 0.9 ± 1.2 −18.6 ± 0.8
γ2 (km s-1) = γ 1 −0.6 ± 1.4 −19.3 ± 0.9
a1 sini (R) 16.53 ± 0.39 17.34 ± 0.13 17.1 ± 0.1
a2 sini (R) 22.17 ± 0.39 22.87 ± 0.17 22.6 ± 0.1
m1 sin3i (M) 14.22 ± 0.64 15.82 ± 0.26 15.2 ± 0.2
m2 sin3i (M) 10.60 ± 0.53 12.00 ± 0.19 11.5 ± 0.2

Notes. Columns 1 and 2 list the orbital solutions from the literature for comparison with our results. The last two columns yield the best-fit parameters accounting for apsidal motion for the full set of 81 RV measurements of the primary star and for the 61 échelle spectra only.

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