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Table 1
Complete V -shape families.
| Designation | Tax. | Dpb | tage,α=1 | tage | N | ac | α | pV | Ds–Dl |
|---|---|---|---|---|---|---|---|---|---|
| (km) | (Gyr) | (Gyr) | (au) | (km) | |||||
| Erigone | C/X | 96.5 | 0.13 ± 0.07 | 0.09 ± 0.04 | 1742 | 2.370 | 0.83 ± 0.05 | 0.05 ± 0.01 | 1.5–23.7 |
| Massalia | S | 145.0 | 0.15 ± 0.07 | 0.19 ± 0.10 | 6414 | 2.410 | 0.73 ± 0.06 | 0.24 ± 0.07 | 0.4–10.8 |
| Misa(2) | C | 27 | 0.13 ± 0.06 | 0.12 ± 0.06 | 427 | 2.655 | 0.87 ± 0.11 | 0.1 ± 0.06 | 2.3–10.0 |
| Tamara | C | 106.0 | 0.18 ± 0.09 | 0.12 ± 0.06 | 111 | 2.310 | 0.7 ± 0.04 | 0.06 ± 0.02 | 1.7–9.8 |
Notes. Diameters for the parent body, Dpb, were taken from the means of asteroid family parent bodies in Brož et al. (2013) and Durda et al. (2007) if Dpb was available from both sources. The estimate of the Tamara parent body size was taken from Novaković et al. (2017).
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