Spin rates of V-type asteroids | Astronomy & Astrophysics (A&A)

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Table A.3

As in Table A.2, but for the fugitive population.

Asteroid	Synodic period	U-code	Diameter	Class,	a	e	sin(i)
No.	(LCDB) (h)	(LCDB)	(km)	references	(au)
809	15.4142	3	9.5	V^{(1,4,15,17,19)}	2.283	0.145	0.1179
956	16.492	3	10.5	V^{(1,4,15,17,19)}	2.298	0.158	0.1119
2049	8.91	2	2.5	V	1.949	0.074	0.4109
2486	4.4518	3	7.9	V^(8,10,13,18)	2.268	0.122	0.1410
2579	3.63599	3	4.6	V^{(1,5,15,16,17)}	2.210	0.082	0.1054
2912	5.71076	3	6.5	V^(1,15,16,17)	2.289	0.118	0.1186
3307	4.902	3−	3.6	V^(1,15)	2.259	0.100	0.1212
3850	2.4289	3	4.2	V^(1,15)	2.235	0.105	0.0814
4692	2.736	2+	4.9	V	2.256	0.122	0.0505
5037	2.8290	−	5.7	QV,V	2.273	0.143	0.1282
5235	2.4524	−	6.7	V^(2,12,14)	2.297	0.120	0.0961
5525	14.088	3−	5.3	V^(2,7,14)	2.221	0.081	0.1279
5560	7.732	3−	4.7	V^(2,7,14)	2.286	0.118	0.0852
5754	8.9021	3	6.3	V	2.267	0.091	0.0843
5952	4.512546	3	4.9	V^{(2,11,13,14,18)}	2.270	0.141	0.0796
6406	6.819	3	4.1	V^(8,9,13,18)	2.276	0.124	0.1336
6819	2.7249	−	4.7	V	2.294	0.102	0.0975
7558	4.1121	−	4.4	V^(2,3,6,14)	2.290	0.110	0.0904
8761	2.6386	−	3.7	V^(2,9,14)	2.242	0.096	0.0639
9481	3.0519	−	4.7	V^(2,14,17)	2.287	0.139	0.036
9531	2.5003	−	4.2	V^(2,7,17,14)	2.235	0.136	0.0957
10666	3.4947	3−	4.0	V^(2,11,14)	2.222	0.110	0.0934
14322	7.462	3	3.5	V^(2,7,14)	2.234	0.106	0.1283
15882	5.05	2	3.8	V	2.297	0.175	0.0419
16416	36.506	2	3.4	V^(2,14,17)	2.196	0.107	0.1079
17028	12.80411	2	2.0	V	2.226	0.152	0.0758
22113	6.7426	−	2.9	V	2.239	0.121	0.0958
23615	368.	2	3.5	V	1.961	0.114	0.3890
26433	7.933	2	2.6	V	2.264	0.110	0.1252
32008	3.0171	3	3.1	V	2.192	0.144	0.1221
37142	47.068	2	1.5	V	2.229	0.122	0.1147
48635	28.106	2	2.4	V	2.266	0.107	0.1034
70069	6.252	2	1.7	V	2.231	0.105	0.1073
84975	22.711	2	1.4	V	2.293	0.126	0.1149
187060	8.125	2	1.0	V	2.241	0.097	0.1318

Notes. In bold, we flag asteroids for which we determined or confirmed periods in this article.

References.⁽¹⁾ Neese (2010), ⁽²⁾ Hasselmann et al. (2012), ⁽³⁾ Wisniewski (1991), ⁽⁴⁾ Florczak et al. (2002), ⁽⁵⁾ Oszkiewicz et al. (2019), ⁽⁶⁾ Moskovitz et al. (2008b), ⁽⁷⁾ Solontoi et al. (2012), ⁽⁸⁾ Alvarez-Candal et al. (2006), ⁽⁹⁾Sanctis et al. (2011), ⁽¹⁰⁾Fulvio et al. (2016), ⁽¹¹⁾Hardersen et al. (2018), ⁽¹²⁾Hardersen et al. (2014b), ⁽¹³⁾Licandro et al. (2017), ⁽¹⁴⁾Carvano et al. (2010), ⁽¹⁵⁾Bus & Binzel (2002), ⁽¹⁶⁾DeMeo et al. (2009), ⁽¹⁷⁾Moskovitz et al. (2010), ⁽¹⁸⁾Popescu et al. (2018), ⁽¹⁹⁾Lazzaro et al. (2004), ⁽²⁰⁾Solontoi et al. (2012).

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