dc.creatorBrunini, Adrián
dc.date2002-11
dc.date2021-08-27T16:13:18Z
dc.date.accessioned2023-07-15T02:55:27Z
dc.date.available2023-07-15T02:55:27Z
dc.identifierhttp://sedici.unlp.edu.ar/handle/10915/123645
dc.identifierissn:0004-6361
dc.identifierissn:1432-0746
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/7463784
dc.descriptionIn 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 combined mean motion resonances with Uranus and Neptune of the form kn<sub>N</sub> + jn<sub>U</sub> + mn ∼ 0 may increase the area of a very thin primordial disk in this region by a factor of up to 2 after 4.5 Gy of evolution.
dc.descriptionFacultad de Ciencias Astronómicas y Geofísicas
dc.descriptionInstituto de Astrofísica de La Plata
dc.formatapplication/pdf
dc.format1129-1134
dc.languageen
dc.rightshttp://creativecommons.org/licenses/by-nc-sa/4.0/
dc.rightsCreative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
dc.subjectAstronomía
dc.subjectKuiper Belt
dc.subjectcomets: general
dc.subjectsolar system: general
dc.titleDynamics of the Edgeworth-Kuiper Belt beyond 50 AU : Spread of a primordial thin disk
dc.typeArticulo
dc.typeArticulo


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