Formation and evolution of planetary systems in presence of highly inclined stellar perturbers

Astronomy and Astrophysics

Volumn 533, Issue , 2011, Pages

  Batygin, K ^a,b   Morbidelli, A ^a   Tsiganis, K ^c  

^a UNIVERSITÉ CÔTE D'AZUR   (France)

^b CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^c ARISTOTLE UNIVERSITY OF THESSALONIKI   (Greece)

Author keywords

methods: analytical; methods: numerical; planets and satellites: dynamical evolution and stability; planets and satellites: formation

Indexed keywords

ANALYTICAL APPROACH; BINARY STAR; BINARY STELLAR SYSTEMS; BINARY SYSTEMS; DYNAMICAL INSTABILITIES; DYNAMICAL STATE; EXTRA SOLAR PLANETS; GRAVITATIONAL INTERACTION; HIGH VELOCITY; ITS ARCHITECTURE; METHODS: NUMERICALS; METHODS:ANALYTICAL; ORBITAL EXCITATIONS; PERTURBATION THEORY; PHYSICAL PROCESS; PLANET FORMATION; PLANETARY FORMATION; PLANETARY SYSTEM; PLANETS AND SATELLITES; PLANETS AND SATELLITES: FORMATION; PROTOPLANETARY DISKS; TRANSIENT PHASE;

NUMERICAL METHODS; PERTURBATION TECHNIQUES; PLANETS; RESONANCE; RIGID STRUCTURES; SATELLITES; SYSTEMS (METALLURGICAL);

STARS;

EID: 80051717734     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201117193     Document Type: Article

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