Table 3: The 70 orbital solutions (Campbell solutions) passing all consistency tests. The column labelled "Ref.'' provides the reference for the spectroscopic orbit used. In the case where a system is listed in the DMSA/O annex, the column labelled "DMSA'' compares the orbital semi-major axes and the inclinations from the DMSA/O annex and from this work.

HIP		 a0 e i $\omega_1$ $\Omega$ T0 P DMSA Ref.
  (mas)   ($^\circ$) ($^\circ$) ($^\circ$) (JD - (d) ( $a/a_{\rm hip};$  
            2400000)   $i/i_{\rm hip}$)  

677		 7.26 $\pm$ 0.38 0.53 102.7 $\pm$ 9.7 77.5 103.4 $\pm$ 5.8 47374.6 96.7 O(1.12;0.97) Pourbaix (2000)
1349 20.98 $\pm$ 0.56 0.57 74.7 $\pm$ 2.1 4.7 352.3 $\pm$ 3.3 34233.3 411.4 O(1.05;0.93) Bopp et al. (1970)
1955 4.68 $\pm$ 0.25 0.33 108.0 $\pm$ 7.5 18.7 299.0 $\pm$ 8.3 35627.6 115.3 5 Barker et al. (1967)
3504 7.4 $\pm$ 1.3 0.11 107.2 $\pm$ 4.3 79.0 274.5 $\pm$ 4.7 41665.0 1033.0 O(1.04;1.06) Abt & Levy (1978)
6867 5.57 $\pm$ 0.46 0.00 46.3 $\pm$ 4.0 0.0 340.2 $\pm$ 5.2 19544.9 193.8 O(1.13;0.92) Luyten (1936)
7078 7.95 $\pm$ 0.15 0.31 85.6 $\pm$ 4.7 188.2 160.5 $\pm$ 3.7 29000.4 134.1 O(1.28;0.97) Wright & Pugh (1954)
8903 12.5 $\pm$ 1.2 0.88 44.7 $\pm$ 5.0 24.9 77.8 $\pm$ 5.6 44809.1 107.0 O(1.10;1.00) Pourbaix (2000)
8922 8.14 $\pm$ 0.93 0.00 23.6 $\pm$ 1.8 0.0 155.7 $\pm$ 4.1 43521.5 838.0 X Griffin (1981b)
10514 5.1 $\pm$ 1.4 0.06 68 $\pm$ 11 63.0 318 $\pm$ 14 41981.5 1385.0 O(0.95;0.92) Griffin & Radford (1977)
11231 8.09 $\pm$ 0.34 0.29 60.6 $\pm$ 3.7 188.2 200.2 $\pm$ 3.8 37159.1 142.3 O(1.43;2.43) Barker et al. (1967)
12062 10.99 $\pm$ 0.87 0.26 56.8 $\pm$ 4.0 254.6 64.9 $\pm$ 5.8 46440.0 905.0 X Latham et al. (2002)
20935 11.5 $\pm$ 1.1 0.24 16.5 $\pm$ 1.3 127.0 308.3 $\pm$ 3.5 43298.5 238.9 O(1.06;0.83) Griffin et al. (1985)
24419 10.77 $\pm$ 0.59 0.08 51.6 $\pm$ 3.3 275.0 230.7 $\pm$ 3.9 50690.0 803.5 9 Nidever et al. (2002)
26001 5.55 $\pm$ 0.46 0.51 52.2 $\pm$ 5.2 330.0 45.4 $\pm$ 6.6 23108.4 180.9 O(1.21;1.17) Lunt (1924)
30277 9.02 $\pm$ 0.52 0.70 116.3 $\pm$ 4.2 117.1 294.6 $\pm$ 5.0 19915.0 868.8 O(0.94;1.01) Spencer Jones (1928b)
32768 7.15 $\pm$ 0.25 0.09 80.2 $\pm$ 6.1 64.0 2.9 $\pm$ 6.2 20992.8 1066.0 O(0.90;1.00) Spencer Jones (1928a)
34164 8.77 $\pm$ 0.96 0.27 107.4 $\pm$ 8.5 248.9 224.3 $\pm$ 8.0 47859.9 612.3 X Latham et al. (2002)
34608 4.92 $\pm$ 0.31 0.40 64.3 $\pm$ 5.9 103.4 85.6 $\pm$ 6.9 44525.0 113.3 O(1.16;0.72) Beavers & Salzer (1985)
36377 8.32 $\pm$ 0.32 0.17 65.6 $\pm$ 3.3 349.3 0.0 $\pm$ 5.2 20418.6 257.8 O(1.02;0.96) Wilson (1918)
39893 9.9 $\pm$ 1.3 0.21 155.3 $\pm$ 2.2 210.0 193.1 $\pm$ 6.6 48342.0 733.5 X Latham et al. (2002)
40326 10.66 $\pm$ 0.73 0.40 135.2 $\pm$ 1.9 140.0 181.7 $\pm$ 2.7 18060.0 930.0 O(0.98;0.99) Christie (1936)
45075 10.35 $\pm$ 0.42 0.48 61.3 $\pm$ 3.2 349.4 119.2 $\pm$ 3.8 25721.6 1062.4 O(0.92;0.91) Bretz (1961)
47461 4.19 $\pm$ 0.67 0.15 122.0 $\pm$ 8.0 135.4 282.7 $\pm$ 9.7 45464.5 635.4 5 Ginestet et al. (1991)
52085 8.09 $\pm$ 0.62 0.10 125.0 $\pm$ 4.4 270.0 327.5 $\pm$ 6.9 20760.0 1200.0 O(1.36;0.85) Christie (1936)
53240 7.83 $\pm$ 0.93 0.38 134.4 $\pm$ 5.4 301.0 292.4 $\pm$ 6.2 42901.5 1166.0 O(0.90;1.09) Griffin (1980)
57791 7.47 $\pm$ 0.60 0.31 86.5 $\pm$ 6.1 125.1 108.5 $\pm$ 4.8 42352.7 486.7 O(0.97;0.99) Ginestet et al. (1985)
60998 5.99 $\pm$ 0.93 0.30 32.5 $\pm$ 4.4 244.0 205.7 $\pm$ 8.6 42868.0 1703.0 7 Reimers et al. (1988)
61724 8.40 $\pm$ 0.82 0.59 81.5 $\pm$ 6.8 102.5 139.0 $\pm$ 7.0 43304.0 972.4 O(0.84;0.96) Griffin (1981a)
62915 5.35 $\pm$ 0.76 0.32 27.1 $\pm$ 3.3 194.0 40.7 $\pm$ 8.4 43424.5 1027. 9 Griffin (1983)
63406 14.12 $\pm$ 0.47 0.33 81.8 $\pm$ 5.0 65.0 101.3 $\pm$ 4.9 49220.0 710.6 O(0.86;1.01) Griffin (2002b)
65417 12.0 $\pm$ 1.7 0.19 68.9 $\pm$ 4.6 166.0 121.1 $\pm$ 3.7 45497.5 1366.8 O(1.17;1.13) Griffin (1986)
67234 6.45 $\pm$ 0.61 0.13 48.2 $\pm$ 3.8 58.6 280.3 $\pm$ 4.9 24163.0 437.0 O(1.01;0.77) Spencer Jones (1928b)
67927 36.02 $\pm$ 0.56 0.26 115.7 $\pm$ 1.6 326.3 75.2 $\pm$ 1.4 28136.2 494.2 O(1.02;0.99) Bertiau (1957)
67480 7.3 $\pm$ 0.9 0.41 174.0 $\pm$ 0.5 359 278.8 $\pm$ 5.8 44739.5 944 X Griffin (1985)
69112 5.74 $\pm$ 0.55 0.14 130.2 $\pm$ 3.8 311.8 158.5 $\pm$ 5.3 38901.7 605.8 O(1.00;0.94) Scarfe (1971)
69879 4.65 $\pm$ 0.24 0.57 89.8 $\pm$ 9.1 224.9 347.0 $\pm$ 8.6 40286.0 212.1 O(1.26;1.02) Scarfe & Alers (1975)
72848 16.54 $\pm$ 0.18 0.51 93.4 $\pm$ 4.2 219.0 248.3 $\pm$ 3.6 50203.4 125.4 O(1.16;0.94) Nidever et al. (2002)
73199 6.10 $\pm$ 0.48 0.13 53.3 $\pm$ 4.0 212.0 239.3 $\pm$ 5.5 44419.0 748.9 O(0.85;0.84) Batten & Fletcher (1986)
73440 4.69 $\pm$ 0.47 0.22 43.9 $\pm$ 5.2 10.0 288.5 $\pm$ 6.5 47349.0 467.2 X Latham et al. (2002)
74087 11.2 $\pm$ 1.6 0.83 62.0 $\pm$ 9.0 175.3 82.6 $\pm$ 6.6 48356.6 2567.1 7 Griffin & Eitter (1999)
75379 8.4 $\pm$ 1.3 0.68 52.6 $\pm$ 9.4 339.5 215.5 $\pm$ 7.5 14785.1 226.9 O(1.00;1.07) Jones (1931)
79101 8.65 $\pm$ 0.64 0.47 10.3 $\pm$ 0.7 357.0 148.3 $\pm$ 3.0 40525.2 560.5 O Aikman (1976)
80346 53.0 $\pm$ 1.8 0.67 152.60 $\pm$ 0.95 251.0 286.9 $\pm$ 1.5 51298.0 1366.1 O(1.02;1.03) Nidever et al. (2002)
80686 2.71 $\pm$ 0.44 0.06 16.01 $\pm$ 2.47 274.5 2.1 $\pm$ 6.8 18103.6 12.9 5 Spencer Jones (1928b)
80816 11.37 $\pm$ 0.51 0.55 53.8 $\pm$ 2.3 24.6 341.9 $\pm$ 3.8 15500.4 410.6 O(1.03;1.16) Plummer (1908)
82860 6.58 $\pm$ 0.32 0.21 56.1 $\pm$ 4.0 339.0 228.7 $\pm$ 4.5 39983.6 52.1 O(0.98;0.90) Abt & Levy (1976)
83575 9.11 $\pm$ 0.58 0.22 61.2 $\pm$ 3.5 348.0 19.5 $\pm$ 4.3 46806.0 790.6 O(1.04;1.03) Griffin (1991)
86400 12.71 $\pm$ 0.78 0.23 18.4 $\pm$ 1.1 140.5 274.2 $\pm$ 2.7 47724.9 83.7 O(0.92;0.41) Tokovinin (1991)
87895 29.81 $\pm$ 0.62 0.41 72.7 $\pm$ 1.2 134.8 177.4 $\pm$ 1.0 47714.6 881.8 O(1.09;1.07) Pourbaix (2000)
88788 10.09 $\pm$ 1.04 0.378 153.9 $\pm$ 2.3 137.0 341.4 $\pm$ 5.8 46139.0 2017.0 9 Griffin (1992)
89937 50.30 $\pm$ 0.23 0.41 80.08 $\pm$ 0.70 119.9 232.42 $\pm$ 0.83 46005.6 280.5 O(1.25;1.07) Pourbaix (2000)
90659 9.1 $\pm$ 1.1 0.50 142.1 $\pm$ 3.0 56.0 353.1 $\pm$ 6.0 42925.5 1284.0 O(0.97;1.01) Griffin (1980)
91751 6.41 $\pm$ 0.53 0.21 59.5 $\pm$ 4.9 78.0 295.8 $\pm$ 7.0 42928.5 485.3 O(1.05;1.05) Griffin (1982b)
92512 3.16 $\pm$ 0.25 0.11 106 $\pm$ 11 274.3 0 $\pm$ 37 19258.2 138.4 O(1.02;1.09) Young (1920)
93244 12.80 $\pm$ 0.44 0.27 87.5 $\pm$ 6.6 82.0 58.7 $\pm$ 3.9 41718.5 1270.6 O(0.94;1.00) Griffin (1982b)
95028 3.0 $\pm$ 0.7 0.37 19 $\pm$ 4 161 242.9 $\pm$ 10.0 43811.9 208.8 7 Griffin (1982b)
95066 9.15 $\pm$ 0.54 0.83 75.2 $\pm$ 8.6 152.7 129.7 $\pm$ 6.7 33420.2 266.5 O(1.18-1.05) Franklin (1952)
95575 8.14 $\pm$ 0.25 0.15 98.2 $\pm$ 7.8 63.3 208.1 $\pm$ 5.7 47746.4 166.4 X Tokovinin (1991)
99848 5.5 $\pm$ 1.2 0.30 65.5 $\pm$ 8.3 218.2 0 $\pm$ 227 33141.8 1147.8 O(1.04;1.02) Wright (1970)
99965 14.06 $\pm$ 0.39 0.08 92.2 $\pm$ 3.6 243.0 303.9 $\pm$ 4.5 50218.0 418.8 O(0.87;0.94) Griffin (2002a)
100437 5.35 $\pm$ 0.57 0.76 54.2 $\pm$ 6.4 108.1 249.7 $\pm$ 8.2 49281.0 1124.1 9 Griffin & Eitter (2000)
101093 19.79 $\pm$ 0.55 0.03 104.0 $\pm$ 1.6 83.7 95.4 $\pm$ 1.7 16214.5 840.6 O(1.39;1.01) Abt (1961)
101847 3.82 $\pm$ 0.81 0.0 147.7 $\pm$ 5.9 0.0 314.0 $\pm$ 1.3 23358.0 205.2 5 Lucy & Sweeney (1971)
103519 7.48 $\pm$ 0.64 0.44 32.4 $\pm$ 2.4 148.1 306.2 $\pm$ 4.0 39186.1 635.1 O(1.02;0.94) Radford & Griffin (1975)
105969 10.65 $\pm$ 0.75 0.13 157.0 $\pm$ 1.3 192.0 236.6 $\pm$ 3.9 47479.0 878.0 X McClure (1997)
109176 4.07 $\pm$ 0.27 0.00 80 $\pm$ 13 0.0 188 $\pm$ 11 45320.0 10.2 5 Fekel & Tomkin (1983)
111170 26.67 $\pm$ 0.73 0.38 63.4 $\pm$ 1.7 171.6 82.0 $\pm$ 1.9 43995.0 630.1 O(1.14;1.07) Pourbaix (2000)
112158 15.62 $\pm$ 0.85 0.15 72.7 $\pm$ 1.9 5.6 208.6 $\pm$ 2.3 15288.7 818.0 O(1.15;1.03) Crawford (1901)
113718 12.16 $\pm$ 0.93 0.54 24.3 $\pm$ 1.8 247.7 328.6 $\pm$ 5.6 48280.0 468.1 O(1.10;0.41) Latham et al. (2002)
114421 7.82 $\pm$ 0.47 0.66 114.3 $\pm$ 5.2 240.8 120.8 $\pm$ 7.2 16115.6 409.6 O(1.26;0.93) Spencer Jones (1928b)


Source LaTeX | All tables | In the text

Article Contents
1 Introduction
2 The Hipparcos data
3 The sample
4 Astrometric wobble detection
5 Orbit assessment
6 Some astrophysical implications
7 Conclusions
References
List of tables
List of figures