Strength, stability and three dimensional structure of mean motion resonances in the solar system
Author:
Funder
CSIC
Publisher
Elsevier BV
Subject
Space and Planetary Science,Astronomy and Astrophysics
Reference36 articles.
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4. Why Halley-types resonate but long-period comets don’t: a dynamical distinction between short- and long-period comets;Chambers;Icarus,1997
5. The origin of long-lived asteroids in the 2:1 mean-motion resonance with Jupiter;Chrenko;MNRAS,2015
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