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Fig. 12

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Scatter plot of the median values of s2 − m (s2 described in Fig. 2 and m in Eq. (1)) and the 0.7 µm band depth for the primitive families that have 5 or more asteroids with computed s2 and band depth bigger than zero (Adeona: 12, Chloris: 5, Mitidika: 5, Themis: 35, Meliboea: 11, and Alauda 15). The size of the crosses is the dispersion of the values of the families.

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