Dynamics of the Edgeworth-Kuiper Belt beyond 50 AU : Spread of a primordial thin disk
In this paper we report numerical simulations of the dynamical evolution of the region a > 50 AU. We found that some dynamical effects such as high-order secular resonances with the rate of precession of Neptune's node of the form kΩ· − Ω·<sub>Nep</sub> with k = 4,5, ... or combi...
Guardado en:
Autor principal: | Brunini, Adrián |
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Formato: | Articulo |
Lenguaje: | Inglés |
Publicado: |
2002
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Materias: | |
Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/123645 |
Aporte de: |
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