Table 1: The 282 stars flagged as astrometric binaries ( Pr₁, Pr₂, Pr₃ < 0.05 and $F2_{{\rm TI}}< 2.37$ ; see text). Italicized entries identify the 122 stars passing the Pr₁, Pr₂ and Pr₃ tests at the more stringent 0.006% level, and $F2_{{\rm TI}}< 2.37$ .
HIP HIP HIP HIP HIP HIP HIP HIP HIP HIP HIP HIP HIP

443 7564 13055 22961 31681 43346 52419 60292 73440 81170 92112 99089 109176

677 7719 14273 23402 32713 43413 52444 60998 74087 82706 92175 99675 109554

1349 8645 15394 23453 32761 43557 52650 61724 75379 82860 92177 99848 110130

1955 8903 15900 23743 32768 43903 52958 62437 75695 83575 92512 99965 110273

2081 8922 16369 23922 33420 44124 53238 62915 75718 83947 92614 100384 110514

2865 9110 17136 23983 34164 44455 53240 63406 76267 84677 92872 100437 111104

3300 9121 17296 24419 34608 44946 53425 63592 76574 84886 92818 100738 111170

3362 10340 17440 24984 35412 45075 53763 64422 76600 84949 92872 101093 111191

3504 10514 17683 25048 36042 45333 54632 65417 77409 85829 93244 101780 112158

3572 10644 17932 25776 36377 46005 55016 65522 77634 85985 94371 101847 113718

3951 10723 18782 26001 36429 46613 55022 67195 77678 86400 95028 102388 113860

4166 11231 19248 26291 37908 46893 56731 67234 77801 86722 95066 103519 114313

4252 11349 20070 27246 38414 47205 57791 67480 78689 87895 95176 103722 114421

4584 11380 20087 28537 39341 47461 58590 67927 79101 88788 95575 103987 116478

4754 11465 20284 29276 39424 49561 59148 68072 79195 88946 95820 105017 116727

4843 11843 20482 29740 39893 49841 59459 68682 79358 89773 95823 105432 117229

5336 11923 20935 29982 40240 50005 59468 69112 80042 89808 96467 105860 117317

5881 12062 21123 30277 40326 50801 59551 69879 80166 89937 97150 105969 117607

6867 12472 21433 30338 41784 50966 59609 69929 80346 90098 97446 106267

7078 12709 21673 30501 42327 51157 59856 72848 80686 90135 97456 107136

7145 12716 21727 31205 42542 52085 60061 72939 80816 90659 97594 108473

7487 12719 22407 31646 42673 52271 60129 73199 81023 91751 98039 109067

**Table 1:** The 282 stars flagged as astrometric binaries ( Pr₁, Pr₂, Pr₃ < 0.05 and $F2_{{\rm TI}}< 2.37$ ; see text). Italicized entries identify the 122 stars passing the Pr₁, Pr₂ and Pr₃ tests at the more stringent 0.006% level, and $F2_{{\rm TI}}< 2.37$ .
HIP	HIP	HIP	HIP	HIP	HIP	HIP	HIP	HIP	HIP	HIP	HIP	HIP
443	7564	13055	22961	31681	43346	52419	60292	73440	81170	92112	99089	109176
677	7719	14273	23402	32713	43413	52444	60998	74087	82706	92175	99675	109554
1349	8645	15394	23453	32761	43557	52650	61724	75379	82860	92177	99848	110130
1955	8903	15900	23743	32768	43903	52958	62437	75695	83575	92512	99965	110273
2081	8922	16369	23922	33420	44124	53238	62915	75718	83947	92614	100384	110514
2865	9110	17136	23983	34164	44455	53240	63406	76267	84677	92872	100437	111104
3300	9121	17296	24419	34608	44946	53425	63592	76574	84886	92818	100738	111170
3362	10340	17440	24984	35412	45075	53763	64422	76600	84949	92872	101093	111191
3504	10514	17683	25048	36042	45333	54632	65417	77409	85829	93244	101780	112158
3572	10644	17932	25776	36377	46005	55016	65522	77634	85985	94371	101847	113718
3951	10723	18782	26001	36429	46613	55022	67195	77678	86400	95028	102388	113860
4166	11231	19248	26291	37908	46893	56731	67234	77801	86722	95066	103519	114313
4252	11349	20070	27246	38414	47205	57791	67480	78689	87895	95176	103722	114421
4584	11380	20087	28537	39341	47461	58590	67927	79101	88788	95575	103987	116478
4754	11465	20284	29276	39424	49561	59148	68072	79195	88946	95820	105017	116727
4843	11843	20482	29740	39893	49841	59459	68682	79358	89773	95823	105432	117229
5336	11923	20935	29982	40240	50005	59468	69112	80042	89808	96467	105860	117317
5881	12062	21123	30277	40326	50801	59551	69879	80166	89937	97150	105969	117607
6867	12472	21433	30338	41784	50966	59609	69929	80346	90098	97446	106267
7078	12709	21673	30501	42327	51157	59856	72848	80686	90135	97456	107136
7145	12716	21727	31205	42542	52085	60061	72939	80816	90659	97594	108473
7487	12719	22407	31646	42673	52271	60129	73199	81023	91751	98039	109067

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