Please use this identifier to cite or link to this item: https://research.matf.bg.ac.rs/handle/123456789/1202
Title: Families among high-inclination asteroids
Authors: Novaković, Bojan 
Cellino, Alberto
Knežević, Zoran
Affiliations: Astronomy 
Keywords: Asteroids;Asteroids, Dynamics;Collisional physics
Issue Date: 1-Nov-2011
Journal: Icarus
Abstract: 
We present a new classification of families identified among the population of high-inclination asteroids. We computed synthetic proper elements for a sample of 18,560 numbered and multi-opposition objects having sine of proper inclination greater than 0.295. We considered three zones at different heliocentric distances (inner, intermediate and outer region) and used the standard approach based on the Hierarchical Clustering Method (HCM) to identify families in each zone. In doing so, we used slightly different approach with respect to previously published methodologies, to achieve a more reliable and robust classification. We also used available SDSS color data to improve membership and identify likely family interlopers. We found a total of 38 families, as well as a significant number of clumps and clusters deserving further investigation. © 2011 Elsevier Inc.
URI: https://research.matf.bg.ac.rs/handle/123456789/1202
ISSN: 00191035
DOI: 10.1016/j.icarus.2011.08.016
Appears in Collections:Research outputs

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