Bojan Novaković

TL;DR: A new approach to the asteroid family classification by combining the Hierarchical Clustering Method (HCM) with a method to add new members to existing families, which allows to solve some difficult cases of families overlapping in the proper elements space but generated by different collisional events.

TL;DR: The main-belt asteroid (300163) 2006 VW139 (later designated P/2006 VW139) was discovered to exhibit comet-like activity by the Pan-STARRS1 (PS1) survey telescope using automated point-spread-function analyses performed by PS1's Moving Object Processing System as mentioned in this paper.

TL;DR: In this article, the authors present observations of the recently discovered comet-like main-belt object P/2010 R2 (La Sagra) obtained by Pan-STARRS1 and the Faulkes Telescope-North on Haleakala in Hawaii, the University of Hawaii 2.2 m, Gemini-North, and Keck I telescopes on Mauna Kea, the Danish 1.54 m telescope (operated by the MiNDSTEp consortium) at La Silla, and the Isaac Newton Telescope on La Palma.

TL;DR: In this paper, a new classification of families identified among the population of high-inclination asteroids was presented, using synthetic proper elements for a sample of 18,560 numbered and multi-opposition objects having sine of proper inclination greater than 0.295.

TL;DR: In this paper, a catalog of accurate synthetic proper elements is used to study the dynamical and collisional evolution of the Hungaria asteroids, and they find a complex interaction between secular resonances, mean motion resonances and chaotic behavior and Yarkovsky-driven drift in semimajor axis.