Table 4: The 31 new orbital solutions (Campbell solutions) passing the Pr₁, Pr₂ and Pr₃ tests at the 0.006% level, but failing at least one of the consistency tests. The column labelled "Ref.'' provides the reference for the spectroscopic orbit used. The columns labelled $\xi$ and $\epsilon$ provide the values of the corresponding empirical tests. The column labelled "D'' refers to DMSA.
HIP a₀ e i $\omega_1$ $\Omega$ T₀ P D $\xi$ $\epsilon$ Ref.

(mas) ( $^\circ$ ) ( $^\circ$ ) ( $^\circ$ ) (JD - (d)

2 400 000)

2081 103.5 $\pm$ 8.2 0.34 128.0 $\pm$ 5.4 19.8 242.8 $\pm$ 3.9 16201.8 3848.8 7 4.25 0.01 Lunt (1924)

5881 7.7 $\pm$ 1.6 0.12 157.2 $\pm$ 4.1 313 236.8 $\pm$ 8.1 51791.1 701.4 5 1.91 0.42 Nidever et al. (2002)

11349 84.4 $\pm$ 4.5 0.01 115.8 $\pm$ 5.0 225. 44.4 $\pm$ 8.2 45901. 3600. 9 3.31 0.07 Latham et al. (2002)

11923 33 $\pm$ 32 0.54 86.2 $\pm$ 24.6 259.0 83 $\pm$ 20 47774.2 2332. 7 4.39 0.07 Latham et al. (2002)

13055 8.12 $\pm$ 0.77 0.09 85.0 $\pm$ 13.7 120 279 $\pm$ 16 46344 2018 7 4.41 0.34 McClure & Woodsworth (1990)

15394 21.9 $\pm$ 3.0 0.86 137.2 $\pm$ 5.9 71.7 81 $\pm$ 10 51190.3 3089.4 7 2.18 0.11 Latham et al. (2002)

27246 56.3 $\pm$ 6.8 0.32 49.6 $\pm$ 7.2 318.5 344.6 $\pm$ 4.4 49649. 4072. 9 5.11 0.02 Latham et al. (2002)

31681 78.7 $\pm$ 2.3 0.89 106.7 $\pm$ 1.7 312.6 243.6 $\pm$ 2.6 43999.1 4614.5 X 2.61 0.01 Lehmann et al. (2002)

38414 32.7 $\pm$ 2.2 0.38 41.3 $\pm$ 1.9 170. 148.5 $\pm$ 3.6 17031. 2554.0 9 5.17 0.10 Parsons (1983)

39424 19.5 $\pm$ 2.9 0.06 50.8 $\pm$ 8.4 264. 242.6 $\pm$ 5.5 42894.5 2437.8 7 2.78 0.11 Griffin (1982a)

43903 37 $\pm$ 3422 0.70 84 $\pm$ 33 194.1 184 $\pm$ 21 49093.7 1898.7 7 5.67 0.05 Carney et al. (2001)

44946 10.5 $\pm$ 1.7 0.06 144.1 $\pm$ 4.9 301.1 282.0 $\pm$ 9.7 28876.8 1700.7 7 2.88 0.28 Jackson et al. (1957)

46893 4.69 $\pm$ 0.77 0.15 132.3 $\pm$ 6.8 261. 2 $\pm$ 11 43119.5 830.4 X 2.84 0.86 Griffin (1981b)

51157 17.9 $\pm$ 1.2 0.86 122.4 $\pm$ 5.2 296.1 255.7 $\pm$ 5.5 44583.0 1180.6 9 2.78 0.41 Griffin (1987)

53238 29.6 $\pm$ 5.0 0.16 143.5 $\pm$ 5.3 285. 221.2 $\pm$ 7.0 45781. 1841. 7 2.73 0.21 Latham et al. (2002)

55016 19.0 $\pm$ 3.1 0.41 53.6 $\pm$ 7.3 336.5 287 $\pm$ 10 42054. 2962.7 7 3.00 0.15 Wolff (1974)

60061 19.6 $\pm$ 2.7 0.41 51.3 $\pm$ 7.7 302.6 11.8 $\pm$ 8.2 50134. 2167. 7 3.33 0.28 Latham et al. (2002)

68072 10.8 $\pm$ 2.7 0.68 20.9 $\pm$ 4.1 177.6 6 $\pm$ 10 47179.1 1620.3 7 4.43 0.32 Latham et al. (2002)

75718 38.6 $\pm$ 1.0 0.97 60.3 $\pm$ 1.8 253.9 95.8 $\pm$ 3.5 47967.5 889.6 7 3.20 0.29 Duquennoy et al. (1992)

79358 16.5 $\pm$ 2.3 0.6 46.4 $\pm$ 3.5 340. 305.4 $\pm$ 6.7 24290. 2150. 7 4.73 0.18 Christie (1936)

84949 24.0 $\pm$ 1.1 0.67 70.2 $\pm$ 3.2 40.0 150.4 $\pm$ 2.1 44545.8 2018.8 X 4.31 0.30 Scarfe et al. (1994)

86722 49.4 $\pm$ 8.5 0.93 41.6 $\pm$ 7.6 129.6 315 $\pm$ 11 49422.5 2558.4 7 3.50 0.01 Duquennoy et al. (1996)

90098 30.7 $\pm$ 4.1 0.26 56.0 $\pm$ 7.0 187.2 54.6 $\pm$ 8.4 18076.2 2214. 9 3.23 0.06 Spencer Jones (1928b)

90135 21.6 $\pm$ 1.9 0.10 89 $\pm$ 16.5 242.1 226 $\pm$ 14 18278.3 2373.7 7 2.85 0.13 Grobben & Michaelis (1969)

92872 26.6 $\pm$ 3.4 0.24 31.9 $\pm$ 3.6 35. 12.6 $\pm$ 7.7 44276.5 2994. 7 3.53 0.04 Griffin (1981b)

94371 33.9 $\pm$ 3.8 0.19 135.5 $\pm$ 5.4 103. 126.9 $\pm$ 6.1 41044.5 2561. 7 3.52 0.09 Griffin (1979)

103987 10.7 $\pm$ 2.7 0.08 162.1 $\pm$ 2.3 83. 15.6 $\pm$ 3.9 46639.0 377.8 9 2.34 0.23 Latham et al. (1992)

114313 17.2 $\pm$ 2.2 0.22 20.2 $\pm$ 1.9 237. 75.1 $\pm$ 4.8 46444. 1132. 9 3.31 0.38 Latham et al. (2002)

116478 20.9 $\pm$ 1.1 0.33 109.8 $\pm$ 6.8 304.3 129.1 $\pm$ 7.8 47403. 1810. 9 4.60 0.16 Latham et al. (2002)

116727 376 $\pm$ 23189 0.38 86 $\pm$ 47 166.0 16 $\pm$ 19 48625 24135 7 5.56 0.01 Griffin et al. (2002)

117229 9.38 $\pm$ 0.78 0.52 102 $\pm$ 12 192.3 251.7 $\pm$ 8.4 48425.8 1756.0 7 2.93 0.59 Latham et al. (2002)

**Table 4:** The 31 new orbital solutions (Campbell solutions) passing the Pr₁, Pr₂ and Pr₃ tests at the 0.006% level, but failing at least one of the consistency tests. The column labelled "Ref.'' provides the reference for the spectroscopic orbit used. The columns labelled $\xi$ and $\epsilon$ provide the values of the corresponding empirical tests. The column labelled "D'' refers to DMSA.
HIP	a₀	e	i	$\omega_1$	$\Omega$	T₀	P	D	$\xi$	$\epsilon$	Ref.
	(mas)		( $^\circ$ )	( $^\circ$ )	( $^\circ$ )	(JD -	(d)
						2 400 000)
2081	103.5 $\pm$ 8.2	0.34	128.0 $\pm$ 5.4	19.8	242.8 $\pm$ 3.9	16201.8	3848.8	7	4.25	0.01	Lunt (1924)
5881	7.7 $\pm$ 1.6	0.12	157.2 $\pm$ 4.1	313	236.8 $\pm$ 8.1	51791.1	701.4	5	1.91	0.42	Nidever et al. (2002)
11349	84.4 $\pm$ 4.5	0.01	115.8 $\pm$ 5.0	225.	44.4 $\pm$ 8.2	45901.	3600.	9	3.31	0.07	Latham et al. (2002)
11923	33 $\pm$ 32	0.54	86.2 $\pm$ 24.6	259.0	83 $\pm$ 20	47774.2	2332.	7	4.39	0.07	Latham et al. (2002)
13055	8.12 $\pm$ 0.77	0.09	85.0 $\pm$ 13.7	120	279 $\pm$ 16	46344	2018	7	4.41	0.34	McClure & Woodsworth (1990)
15394	21.9 $\pm$ 3.0	0.86	137.2 $\pm$ 5.9	71.7	81 $\pm$ 10	51190.3	3089.4	7	2.18	0.11	Latham et al. (2002)
27246	56.3 $\pm$ 6.8	0.32	49.6 $\pm$ 7.2	318.5	344.6 $\pm$ 4.4	49649.	4072.	9	5.11	0.02	Latham et al. (2002)
31681	78.7 $\pm$ 2.3	0.89	106.7 $\pm$ 1.7	312.6	243.6 $\pm$ 2.6	43999.1	4614.5	X	2.61	0.01	Lehmann et al. (2002)
38414	32.7 $\pm$ 2.2	0.38	41.3 $\pm$ 1.9	170.	148.5 $\pm$ 3.6	17031.	2554.0	9	5.17	0.10	Parsons (1983)
39424	19.5 $\pm$ 2.9	0.06	50.8 $\pm$ 8.4	264.	242.6 $\pm$ 5.5	42894.5	2437.8	7	2.78	0.11	Griffin (1982a)
43903	37 $\pm$ 3422	0.70	84 $\pm$ 33	194.1	184 $\pm$ 21	49093.7	1898.7	7	5.67	0.05	Carney et al. (2001)
44946	10.5 $\pm$ 1.7	0.06	144.1 $\pm$ 4.9	301.1	282.0 $\pm$ 9.7	28876.8	1700.7	7	2.88	0.28	Jackson et al. (1957)
46893	4.69 $\pm$ 0.77	0.15	132.3 $\pm$ 6.8	261.	2 $\pm$ 11	43119.5	830.4	X	2.84	0.86	Griffin (1981b)
51157	17.9 $\pm$ 1.2	0.86	122.4 $\pm$ 5.2	296.1	255.7 $\pm$ 5.5	44583.0	1180.6	9	2.78	0.41	Griffin (1987)
53238	29.6 $\pm$ 5.0	0.16	143.5 $\pm$ 5.3	285.	221.2 $\pm$ 7.0	45781.	1841.	7	2.73	0.21	Latham et al. (2002)
55016	19.0 $\pm$ 3.1	0.41	53.6 $\pm$ 7.3	336.5	287 $\pm$ 10	42054.	2962.7	7	3.00	0.15	Wolff (1974)
60061	19.6 $\pm$ 2.7	0.41	51.3 $\pm$ 7.7	302.6	11.8 $\pm$ 8.2	50134.	2167.	7	3.33	0.28	Latham et al. (2002)
68072	10.8 $\pm$ 2.7	0.68	20.9 $\pm$ 4.1	177.6	6 $\pm$ 10	47179.1	1620.3	7	4.43	0.32	Latham et al. (2002)
75718	38.6 $\pm$ 1.0	0.97	60.3 $\pm$ 1.8	253.9	95.8 $\pm$ 3.5	47967.5	889.6	7	3.20	0.29	Duquennoy et al. (1992)
79358	16.5 $\pm$ 2.3	0.6	46.4 $\pm$ 3.5	340.	305.4 $\pm$ 6.7	24290.	2150.	7	4.73	0.18	Christie (1936)
84949	24.0 $\pm$ 1.1	0.67	70.2 $\pm$ 3.2	40.0	150.4 $\pm$ 2.1	44545.8	2018.8	X	4.31	0.30	Scarfe et al. (1994)
86722	49.4 $\pm$ 8.5	0.93	41.6 $\pm$ 7.6	129.6	315 $\pm$ 11	49422.5	2558.4	7	3.50	0.01	Duquennoy et al. (1996)
90098	30.7 $\pm$ 4.1	0.26	56.0 $\pm$ 7.0	187.2	54.6 $\pm$ 8.4	18076.2	2214.	9	3.23	0.06	Spencer Jones (1928b)
90135	21.6 $\pm$ 1.9	0.10	89 $\pm$ 16.5	242.1	226 $\pm$ 14	18278.3	2373.7	7	2.85	0.13	Grobben & Michaelis (1969)
92872	26.6 $\pm$ 3.4	0.24	31.9 $\pm$ 3.6	35.	12.6 $\pm$ 7.7	44276.5	2994.	7	3.53	0.04	Griffin (1981b)
94371	33.9 $\pm$ 3.8	0.19	135.5 $\pm$ 5.4	103.	126.9 $\pm$ 6.1	41044.5	2561.	7	3.52	0.09	Griffin (1979)
103987	10.7 $\pm$ 2.7	0.08	162.1 $\pm$ 2.3	83.	15.6 $\pm$ 3.9	46639.0	377.8	9	2.34	0.23	Latham et al. (1992)
114313	17.2 $\pm$ 2.2	0.22	20.2 $\pm$ 1.9	237.	75.1 $\pm$ 4.8	46444.	1132.	9	3.31	0.38	Latham et al. (2002)
116478	20.9 $\pm$ 1.1	0.33	109.8 $\pm$ 6.8	304.3	129.1 $\pm$ 7.8	47403.	1810.	9	4.60	0.16	Latham et al. (2002)
116727	376 $\pm$ 23189	0.38	86 $\pm$ 47	166.0	16 $\pm$ 19	48625	24135	7	5.56	0.01	Griffin et al. (2002)
117229	9.38 $\pm$ 0.78	0.52	102 $\pm$ 12	192.3	251.7 $\pm$ 8.4	48425.8	1756.0	7	2.93	0.59	Latham et al. (2002)

Source LaTeX | All tables | In the text

	1 Introduction
	2 The Hipparcos data
	3 The sample
	4 Astrometric wobble detection
	5 Orbit assessment
	6 Some astrophysical implications
	7 Conclusions
	References