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Table 2

Astrometric orbits based on the original Hipparcos data with and without spectroscopic help.

Spectro-based
Element Original Tycho-2 Campbell Thiele-Innes

e 0 (fixed) 0.589 (fixed)
P (d) 877.6541 ± 117.3686 1126.11 (fixed)
T0 (JD-2 400 000) 48   589.2621 ± 38.5598 53 766.2 (fixed)
a0 (mas) 5.91 ± 0.93 8.4 ± 0.52 9.8
i (deg) 93.51 ± 5.34 93 ± 4.7 93
ω (deg) 0 (fixed) 201.6 (fixed) 196
Ω (deg) 161.88 ± 6.94 159 ± 6.4 156
A (mas) 8 ± 1.0
B (mas) −4 ± 1.0
F (mas) −2.7 ± 0.80
G (mas) −0.6 ± 0.67
F2 0.10 –0.83 –0.87
K1 (km s-1) 6.93 9.21 (fixed) 11
ϖ (mas) 10.55 ± 0.69 10.87 ± 0.67 10.6 ± 0.69
μα ∗ (mas yr-1) −34.32 ± 0.68 −33.7 ± 0.7 −35.3 ± 0.74 −35.7 ± 0.78
μδ (mas yr-1) −28.34 ± 1.39 −26.0 ± 0.6 −25.8 ± 0.52 −25.4 ± 0.61

Notes.The second column lists the published solution (ESA 1997). As in the Hipparcos Catalogue, F2 denotes the goodness of fit and ϖ the parallax. The third column lists the proper motion after Tycho-2 (Høg et al. 2000).

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