Fig. 5
Proportion of asteroids from each primitive class with respect to the total number of primitive asteroids found for each family. The percentage of asteroids showing the 0.7 μm absorption band within each class is shown in blue. We compare the results obtained for the Sulamitis family (this work, light green) with those obtained in Morate et al. (2016) for the Erigone family (dark green).
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