Circular Restricted Three-body Problem
The Circular Restricted Three-Body Problem is a specialized case of the three-body problem in celestial mechanics in which two massive bodies follow circular orbits around their common center of mass under mutual gravitational attraction, while a third body of negligible mass moves under their influence without perturbing their motion.
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174
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2017–2026
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Crtbp
195
Connecting orbits and invariant manifolds in the spatial restricted three-body problem
Gérard Gómez, Wang Sang Koon, M. W. Lo et al. · Nonlinearity · 2004 · 312 citations
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Universitat Politècnica de Catalunya
Barcelona, Spain
11 h-index
15 publications
736 citations
Aristotle University of Thessaloniki
Thessaloniki, Greece
9 h-index
9 publications
374 citations
University of Patras
Pátrai, Greece
8 h-index
15 publications
410 citations
Jet Propulsion Laboratory
Pasadena, United States
8 h-index
10 publications
553 citations
University of Colorado Boulder
Boulder, United States
6 h-index
4 publications
61 citations
Politecnico di Milano
Milan, Italy
6 h-index
10 publications
500 citations

Ahmadu Bello University
Zaria, Nigeria
6 h-index
8 publications
168 citations
Majmaah University
Riyadh, Saudi Arabia
6 h-index
9 publications
132 citations
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31 publications · 928 citations
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16 publications · 695 citations
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AJ · 10 publications · 764 citations
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9 publications · 375 citations
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7 publications · 187 citations
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