P/2006 VW139: A Main-Belt Comet Born in an Asteroid Collision?
Bojan Novakovic, Henry H. Hsieh, Alberto Cellino

TL;DR
This study investigates the origin of main-belt comet P/2006 VW139 and its associated asteroid family, revealing a recent collision event and providing insights into the activation mechanisms of such comets.
Contribution
The paper presents the first detailed analysis linking P/2006 VW139 to a young asteroid family formed by a recent collision, using multiple dynamical methods.
Findings
Strong evidence for a 11-member asteroid family linked to P/2006 VW139
Estimated family age of approximately 7.5 million years
Family formed by a transition from catastrophic to cratering impact regime
Abstract
In this paper we apply different methods to examine the possibility that a small group of 24 asteroids dynamically linked to main-belt comet P/2006 VW139, recently discovered by the Pan-STARRS1 survey telescope, shares a common physical origin. By applying the Hierarchical Clustering and Backward Integration methods, we find strong evidence that 11 of these asteroids form a sub-group which likely originated in a recent collision event, and that this group includes P/2006 VW139. The objects not found to be part of the 11-member sub-group, which we designate as the P/2006 VW139 family, were either found to be dynamically unstable, or these are likely interlopers which should be expected due to the close proximity of the Themis family. As we demonstrated, statistical significance of P/2006 VW139 family is >99 per cent. We determine the age of the family to be 7.5 +/- 0.3 Myr, and estimate…
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