Image Details
Caption: Figure 3.
Similar to the top panels of Figure 1 but in ﹩1/D-a﹩ (inverse diameter versus proper semimajor axis) space and superimposed by the V-shaped bounding lines. For the Vesta family, bounding lines are obtained by assuming different values for the family age and asteroid mean density (Appendix A3).
© 2026. The Author(s). Published by the American Astronomical Society.