تقرير
Orbital Stability of Planets in Binary Systems: A New Look at Old Results
| العنوان: | Orbital Stability of Planets in Binary Systems: A New Look at Old Results |
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| المؤلفون: | Eberle, J., Cuntz, M., Musielak, Z. E. |
| سنة النشر: | 2007 |
| المجموعة: | Astrophysics |
| مصطلحات موضوعية: | Astrophysics |
| الوصف: | About half of all known stellar systems with Sun-like stars consist of two or more stars, significantly affecting the orbital stability of any planet in these systems. This observational evidence has prompted a large array of theoretical research, including the derivation of mathematically stringent criteria for the orbital stability of planets in stellar binary systems, valid for the "coplanar circular restricted three-body problem". In the following, we use these criteria to explore the validity of results from previous theoretical studies. Comment: 3 pages, 1 figure; submitted to: Exoplanets: Detection, Formation and Dynamics, IAU Symposium 249, eds. Y.-S. Sun, S. Ferraz-Mello, and J.-L. Zhou (Cambridge: Cambridge University Press) |
| نوع الوثيقة: | Working Paper |
| DOI: | 10.1017/S1743921308017043 |
| URL الوصول: | http://arxiv.org/abs/0712.3239 |
| رقم الأكسشن: | edsarx.0712.3239 |
| قاعدة البيانات: | arXiv |
| DOI: | 10.1017/S1743921308017043 |
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