An anisotropic distribution of spin vectors in asteroid families

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Table 2

List of partial models derived from combined data sets.

Asteroid		β	Δ	P	N _lc	N _app	N ₆₈₉	N ₇₀₃
		[deg]	[deg]	[hours]

391	Ingeborg	−60	7	26.4145	24	2	141	96
502	Sigune	−44	3	10.92667	9	2	157	52
616	Elly	67	23	5.29771	4	1	101	133
1003	Lilofee	65	10	8.24991			107	83
1160	Illyria	47	23	4.10295			96	100
1192	Prisma	−65	14	6.55836	5	1	44	43
1276	Ucclia	−49	22	4.90748			114	45
1307	Cimmeria	63	9	2.820723	2	1	91	54
1339	Desagneauxa	65	17	9.37510			78	120
1396	Outeniqua	62	7	3.08175	2	1	112	68
1493	Sigrid	78	7	43.179			78	103
1619	Ueta	39	6	2.717943	5	1	122	51
1623	Vivian	−75	8	20.5235			77	58
1738	Oosterhoff	−72	8	4.44896			109	105
1838	Ursa	47	17	16.1635			102	91
2086	Newell	−60	12	78.09	10	1	24	84
3017	Petrovic	−73	8	4.08037	3	1		114
3786	Yamada	56	2	4.03294	3	1		71
3896	Pordenone	−32	9	4.00366	3	1	22	71
4209	Briggs	−56	25	12.2530	2	1		64
4467	Kaidanovskij	54	13	19.1454			20	107
6179	Brett	−42	20	9.4063	6	1		93
7055	1989 KB	−61	11	4.16878	7	1		117
7360	Moberg	−18	18	4.58533	3	1		103

Notes. For each asteroid, there is the mean ecliptic latitude β of the pole direction and its dispersion Δ. The other parameters have the same meaning as in Table 1. The uncertainty of the sidereal rotational period corresponds to the last decimal place of P.

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