Secondary resonances of co-orbital motions

Monthly Notices of the Royal Astronomical Society

Volumn 381, Issue 1, 2007, Pages 33-40

  Erdi B ^a   Nagy, I ^b   Sandor Zs ^a   Suli A ^a   Frohlich G ^a  

^a EÖTVÖS LORÁND UNIVERSITY   (Hungary)

^b BUDAPEST UNIVERSITY OF TECHNOLOGY AND ECONOMICS   (Hungary)

Author keywords

Celestial mechanics; Methods: numerical; Planetary systems

Indexed keywords

NUMERICAL METHODS; ORBITS; SIZE DISTRIBUTION;

CELESTIAL MECHANICS; LAGRANGIAN POINTS; MASS PARAMETER; METHOD: NUMERICAL; ORBITAL MOTIONS; PLANETARY SYSTEM; RESTRICTED THREE-BODY PROBLEM; SECONDARY RESONANCES; SIZE-DISTRIBUTION; STABILITY REGIONS;

ASTROPHYSICS;

EID: 35148845126     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2007.12228.x     Document Type: Article

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