Secondary resonances and the boundary of effective stability of Trojan motions
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Title
Secondary resonances and the boundary of effective stability of Trojan motions
Authors
Keywords
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Journal
CELESTIAL MECHANICS & DYNAMICAL ASTRONOMY
Volume 130, Issue 2, Pages -
Publisher
Springer Nature
Online
2018-02-14
DOI
10.1007/s10569-017-9814-4
References
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Related references
Note: Only part of the references are listed.- Detection of co-orbital planets by combining transit and radial-velocity measurements
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- (2014) A. Pierens et al. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
- High order normal form stability estimates for co-orbital motion
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- (2013) Anthony R. Dobrovolskis ICARUS
- Where are the Uranus Trojans?
- (2010) R. Dvorak et al. CELESTIAL MECHANICS & DYNAMICAL ASTRONOMY
- Origin and dynamical evolution of Neptune Trojans - II. Long-term evolution
- (2010) P. S. Lykawka et al. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
- Stability of Trojan planets in multi-planetary systems
- (2009) R. Schwarz et al. CELESTIAL MECHANICS & DYNAMICAL ASTRONOMY
- On the growth and stability of Trojan planets
- (2008) P. Cresswell et al. ASTRONOMY & ASTROPHYSICS
- Nekhoroshev stability atL4orL5in the elliptic-restricted three-body problem - application to Trojan asteroids
- (2008) Ch. Lhotka et al. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
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