Dynamical evolution of basaltic asteroids outside the Vesta family in the inner main belt

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Fig. 2

Evolution oſ proper elements of asteroids considered in this work. Black points show the long-term drift (ΔT = −2 Gyr) of proper a, e and i of the objects from Table 3. The red circles mark the current positions and the blue circles mark trie positions of 2 Gyr ago of the objects.

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