Secular evolution of resonant planets in the coplanar case. Application to the systems HD 73526 and HD 31527
Aims. We study the secular evolution of two planets in mutual deep mean-motion resonance (MMR) in the planar elliptic three-body problem framework for different mass ratios. We do not consider any restriction in the eccentricity of the inner planet e1 or in the eccentricity of the outer planet e2. M...
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| Formato: | article |
| Idioma: | inglês |
| Publicado em: |
2024
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| Acesso em linha: | https://hdl.handle.net/20.500.12008/48771 |
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