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pro vyhledávání: '"Hadjidemetriou, John D"'
Over the last decades, there has been a tremendous increase in research on extrasolar planets. Many exosolar systems, which consist of a Star and two inclined Planets, seem to be locked in 4/3, 3/2, 2/1, 5/2, 3/1 and 4/1 mean motion resonance (MMR).
Externí odkaz:
http://arxiv.org/abs/1311.4396
The birth and death of planets may be affected by mass outflows from their parent stars during the T-Tauri or post-main-sequence phases of stellar evolution. These outflows are often modelled to be isotropic, but this assumption is not realistic for
Externí odkaz:
http://arxiv.org/abs/1308.0599
Many exo-solar systems discovered in the last decade consist of planets orbiting in resonant configurations and consequently, their evolution should show long-term stability. However, due to the mutual planetary interactions a multi-planet system sho
Externí odkaz:
http://arxiv.org/abs/1306.0689
Discoveries of exoplanets orbiting evolved stars motivate critical examinations of the dynamics of $N$-body systems with mass loss. Multi-planet evolved systems are particularly complex because of the mutual interactions between the planets. Here, we
Externí odkaz:
http://arxiv.org/abs/1301.5441
We present families of symmetric and asymmetric periodic orbits at the 1/1 resonance, for a planetary system consisting of a star and two small bodies, in comparison to the star, moving in the same plane under their mutual gravitational attraction. T
Externí odkaz:
http://arxiv.org/abs/1105.2713
Publikováno v:
In Icarus 2002 159(2):284-299
Publikováno v:
In Icarus 2002 155(2):454-474
Publikováno v:
In Icarus 2000 146(1):240-252
Publikováno v:
Proceedings of the International Astronomical Union. 08/01/2004, Vol. 2004 Issue IAUC197, p55-62. 8p.
Akademický článek
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