Table 5:

The (circular) orbital solutions based on the 1031-d period.

Element	Solution 1: H emis.	Solution 2: He I 6678
P (d)	1031.55    0.71	1031.55 fixed
	51759.2   1.4	51749.5   4.5
K (km s-1)	21.593    0.071	20.81   0.60
(km s-1)	*)	-12.36   0.41
f(m) ()	1.076	0.9634
rms (km s-1)	0.944	7.42
No. of RVs	437	430

Notes. For the H emission line RVs, the data were divided into five segments, covering individual orbital periods, and treated formally as coming from different spectrographs with different systemic RVs. Thus, we were able to remove the slight long-term variations affecting the RVs. No such procedure was applied to the He I 6678 RVs. All epochs are in HJD-2 400 000; rms is the rms of the O-C values.
^*) Local 's ranged from -5.8 to -11.6 km s^-1, all with rms errors below 1 km s^-1.