On the dynamical evolution and end states of binary centaurs

In this paper,we perform a numerical integration of 666 fictitious binary Centaurs coming from the trans Neptunian space. Our population is restricted to tight binaries whose components have sizes between 30 and 100 km. We included the dynamical perturbations from the giant planets, Kozai Cycles ind...

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Detalles Bibliográficos
Autor principal:	Brunini, Adrián
Formato:	Articulo
Lenguaje:	Inglés
Publicado:	2014
Materias:	Ciencias Astronómicas General - comets General - planetary systems Kuiper belt
Acceso en línea:	http://sedici.unlp.edu.ar/handle/10915/85298
Aporte de:	SEDICI (UNLP) de Universidad Nacional de La Plata

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