Table 6: Masses and mass ratios for the 29 systems with main-sequence primaries passing all consistency tests.
HIP M₁ ( $M_{\odot}$ ) M₂( $M_{\odot}$ ) M₂/M₁ $Q = \frac{M_2^3}{(M_1+M_2)^2}$ Sp. Type Rem.

1349 0.98 0.55 0.56 0.0711 G2

1955 1.13 0.48 0.42 0.0420 GO

7078 1.21 0.70 0.58 0.0953 F6

8903 1.86 1.05 0.56 0.1358 A5

11231 1.01 0.68 0.67 0.111 G2

12062 0.95 0.44 0.47 0.0449 G5

20935 1.13 1.11 0.98 0.2732 F7 not a composite spectrum despite a mass ratio close to unity

24419 0.90 0.21 0.24 0.0079 G8

34164 1.09 0.66 0.61 0.0954 G0

39893 0.95 0.52 0.55 0.0649 G3

47461 - - - 0.0863 F2 composite spectrum

63406 0.82 0.23 0.28 0.0114 G9

72848 0.79 0.45 0.56 0.0581 K2

73440 1.03 0.15 0.14 0.0023 G0

75379 1.26 0.68 0.54 0.0842 F5

79101 3.47 1.31 0.38 0.0976 B9

80346 0.50 0.13 0.26 0.0054 M3

80686 1.05 0.37 0.36 0.0259 G0

82860 1.18 0.52 0.44 0.0482 F6

86400 0.72 0.39 0.54 0.0475 K3

87895 0.99 0.68 0.69 0.1129 G2

89937 1.18 0.77 0.65 0.1195 F7Vvar

95028 1.40 0.50 0.36 0.0353 F5

95575 0.78 0.38 0.49 0.0405 K3

99965 0.88 0.56 0.63 0.0840 G5

105969 1.01 0.49 0.49 0.0528 Dwarf Ba/Subgiant CH

109176 1.25 0.80 0.64 0.1233 F5

111170 1.08 0.70 0.65 0.1083 F7

113718 0.76 0.18 0.24 0.0067 K4

**Table 6:** Masses and mass ratios for the 29 systems with main-sequence primaries passing all consistency tests.
HIP	M₁ ( $M_{\odot}$ )	M₂( $M_{\odot}$ )	M₂/M₁	$Q = \frac{M_2^3}{(M_1+M_2)^2}$	Sp. Type	Rem.
1349	0.98	0.55	0.56	0.0711	G2
1955	1.13	0.48	0.42	0.0420	GO
7078	1.21	0.70	0.58	0.0953	F6
8903	1.86	1.05	0.56	0.1358	A5
11231	1.01	0.68	0.67	0.111	G2
12062	0.95	0.44	0.47	0.0449	G5
20935	1.13	1.11	0.98	0.2732	F7	not a composite spectrum despite a mass ratio close to unity
24419	0.90	0.21	0.24	0.0079	G8
34164	1.09	0.66	0.61	0.0954	G0
39893	0.95	0.52	0.55	0.0649	G3
47461	-	-	-	0.0863	F2	composite spectrum
63406	0.82	0.23	0.28	0.0114	G9
72848	0.79	0.45	0.56	0.0581	K2
73440	1.03	0.15	0.14	0.0023	G0
75379	1.26	0.68	0.54	0.0842	F5
79101	3.47	1.31	0.38	0.0976	B9
80346	0.50	0.13	0.26	0.0054	M3
80686	1.05	0.37	0.36	0.0259	G0
82860	1.18	0.52	0.44	0.0482	F6
86400	0.72	0.39	0.54	0.0475	K3
87895	0.99	0.68	0.69	0.1129	G2
89937	1.18	0.77	0.65	0.1195	F7Vvar
95028	1.40	0.50	0.36	0.0353	F5
95575	0.78	0.38	0.49	0.0405	K3
99965	0.88	0.56	0.63	0.0840	G5
105969	1.01	0.49	0.49	0.0528	Dwarf Ba/Subgiant CH
109176	1.25	0.80	0.64	0.1233	F5
111170	1.08	0.70	0.65	0.1083	F7
113718	0.76	0.18	0.24	0.0067	K4

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