Planetary Dynamics in Binary Systems: A Qualitative Analysis of the S-Type Case

被引：2
|
作者：
Lara, Martin [1 ]
Palacian, Jesus F. [2 ]
Yanguas, Patricia [2 ]
机构：
[1] Real Observ Armada, San Fernando, Spain
[2] Univ Publ Navara, Dep Ingn Matemat Informat, Pamplona, Spain
来源：
INTERNATIONAL WORKSHOP ON DOUBLE AND MULTIPLE STARS: DYNAMICS, PHYSICS, AND INSTRUMENTATION | 2011年 / 1346卷
关键词：
Binary systems; extrasolar planets; Kozai mechanism; perturbation methods; HIGH-INCLINATION; KOZAI MECHANISM; 3-BODY PROBLEM; ORBITS; STABILITY; STARS;
D O I：
10.1063/1.3597588
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The qualitative dynamics of S-type orbits in binary systems is studied in the framework of the three-dimensional Elliptic Restricted Three-Body Problem. A chain of canonical Lie-transforms is applied to reduce stepwise the original, time-dependent system to one of one degree of freedom. Then, the reduced systems are analyzed, computing the relative equilibria of the flows and their stability.
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页数：10
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