**Table 1:** A list of the detected runaway OB star candidates.
HIP	HD/BD	Sp. type	${(v_{\rm t})}_{\rm pec}$	$v_{\rm tr}$	${(v_{\rm t})}_{\rm pec}^*$	HIP	HD/BD	Sp. type	${(v_{\rm t})}_{\rm pec}$	$v_{\rm tr}$	${(v_{\rm t})}_{\rm pec}^*$
			km s^-1	km s^-1	km s^-1				km s^-1	km s^-1	km s^-1
2702	3175	B5III	95.05	62.57		73 720	133 294	B8II	87.21	107.05
4384	5342	B8II	56.60	43.04	10.68	73 778	132 791	B9II/III	83.88	126.20
5778	7374	B8III	62.38	59.47	34.80	74 660	134 959	B2Ia	82.22	98.33
13 489	18 100	B5II/III	131.68	111.01		75 711	137 595	B2II/III	228.81	245.44
14 514	19 374	B1.5V	78.47	67.40	39.79	80 338	147 648	B8II	158.57	171.62	7.16
24 575	34 078	O9.5Vvar	120.19	107.00	103.76	81 153	149 363	B0.5III	145.30	156.09
26 272	36 879	O7.5III	81.47	89.12		81 362	149 881	B0.5III	64.25	48.85
27 204	38 666	B1IV/V	78.81	67.06	51.20	81 696	150 135	O7V	87.34	84.67
29 147	41 997	O7	75.90	84.35		81 904	150 608	B9II/III	66.67	81.17	30.99
29 201	42 259	B0V	85.91	90.20	25.97	82 171	150 898	B0Iab	133.23	162.39
29 317	41 689	B1Vn...	95.29	91.02		82 217	151 346	B8II	104.01	116.06	15.33
29 678	43 112	B1V	98.73	93.49	58.17	82 625	152 160	B8/B9II	95.83	113.49
30 071	44 182	B8II	57.51	42.39		83 509	153 772	B2V	73.35	59.32
31 365	259 954	B2IV	76.21	70.19		87 164	161 653	B2II	59.53	54.83	19.46
34 117	53 269	B9III	145.43	143.53		87 287	162 365	B2IV	61.57	54.52
35 707	57 682	O9V	98.81	96.97		89 902	167 806	B2V	80.85	80.42	40.14
36 243	58 683	B8III	69.61	82.63	59.80	90 074	168 733	B7Ib/II	120.12	133.71	10.28
36 799	60 930	B9II	150.70	198.75	24.29	100 170	192 273	B2V	61.37	74.16
38 184	63 655	B8/B9II	56.20	49.85	33.58	101 350	195 965	B0V	69.63	61.62	31.34
41 603	71 833	B8II	109.38	92.307	39.30	101 729	+45 3230	B0III	68.22	31.64
46 592	82 011	B9III	86.16	93.91		102 999	198 846	B0IVv SB	129.64	159.53
47 370	83 866	B8II	91.20	149.51	11.47	104 361	201 522	B0V	63.74	33.20	7.44
48 128	84 971	B2V	73.15	43.17		105 811	204 172	B0Ib	74.04	79.53
48 715	86 606	B1Ib	194.03	147.28	69.82	106 917	205 805	B7III	935.12	952.91	84.11
54 524	--	B6III	123.87	170.64	17.65	110 266	212 043	B6II	133.41	117.92	17.79
55 051	97 991	B1V	269.90	243.86		111 086	213 236	B8II	213.87	225.26	30.84
57 870	103 101	B4III	142.78	161.30	42.03	111 544	214 168	B2V	60.28	52.33
65 890	116 852	O9Ib	120.80	91.46		111 563	214 080	B1/B2Ib	238.49	255.13
66 524	118 450	B5II	383.90	422.62	108.52	112 022	214 930	B2IV	68.23	71.43
69 640	124 300	B2V	49.80	12.32	18.43	113 735	217 505	B2III/IV	85.50	125.80
						114 998	219 639	B5II/III	98.93	106.94

Notes: Entries are ordered by the increasing HIPPARCOS number of a star. The values for ${(v_{\rm t})}_{\rm pec}^*$ which have
unreliable HIPPARCOS distance estimates (with relative uncertainties more than 50%) are missed.

Source LaTeX | All tables | In the text

	1 Introduction
	2 Estimation of the peculiar tangential velocities and errors in peculiar tangential velocities
	3 Discussion and conclusions
	References