61 citations · 71 across the 2 of their papers we have counts for
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astro-ph.EP2018
Asteroid families interacting with secular resonances
V. Carruba, D. Vokrouhlický, B. Novakovic
Asteroid families are formed as the result of collisions. Large fragments are ejected with speeds of the order of the escape velocity from the parent body. After the family formati…
astro-ph.EP2016★ 10 cited
The Hoffmeister asteroid family
V. Carruba, B. Novakovic, S. Aljbaae
The Hoffmeister family is a C-type group located in the central main belt. Dynamically, it is important because of its interaction with the nodal secular resonance with Ce…
astro-ph.EP2016★ 61 cited
On the Ages of Resonant, Eroded and Fossil Asteroid Families
A. Milani, Z. Knežević, F. Spoto +3
In this work we have estimated 10 collisional ages of 9 families for which for different reasons our previous attempts failed. In general, these are difficult cases that required d…