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Table 3

Orbital solutions for the four newly-detected binary systems.

Parameters HD 193443 HD 228989 HD 229234 HD194649
Primary Secondary Primary Secondary Primary Primary Secondary

P [d] 7.467  ±  0.003 1.77352  ±  0.00041 3.51059  ±  0.00175 3.39294  ±  0.00139
e 0.315  ±  0.024 0.0 0.0 0.0
ω    [°]  289.7  ±  5.8
T0 (HJD) 3246.120  ±  0.106 5047.771  ±  0.003 4714.326  ±  0.011 4991.082  ±  0.009
γ [km s-1]  −10.0  ±  1.2  −16.6  ±  2.0  −3.7  ±  1.8  −7.8  ±  1.9  −16.3  ±  0.8  −13.8  ±  2.1  −29.5  ±  3.1
K [km s-1] 38.8  ±  1.5 91.3  ±  3.4 194.3  ±  2.5 220.3  ±  2.9 48.5  ±  1.1 76.3  ±  2.5 192.1  ±  6.2
a sin i [R] 5.4  ±  0.2 12.8  ±  0.5 6.8  ±  0.1 7.7  ±  0.1 3.4  ±  0.1 5.1  ±  0.2 12.9  ±  0.4
M sin3 i [M] 1.0  ±  0.1 0.4  ±  0.1 7.0  ±  0.2 6.1  ±  0.2 4.9  ±  0.4 1.9  ±  0.1
q (MP/MS) 2.35  ±  0.11 1.13  ±  0.02 2.52  ±  0.13
fmass [M] 0.042  ±  0.003
rms [km s-1] 5.08 8.37 3.04 11.13

Notes. The 1-σ error-bars on the parameters are provided by LOSP, except for the orbital period whose uncertainty is determined on the basis of the natural width of the peaks in the Fourier power spectrum. The orbital solution of HD 193443 was computed assuming that the uncertainties on the secondary RVs are three times as large as for the primary.

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