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dc.date.accessioned 2019-10-11T15:51:51Z
dc.date.available 2019-10-11T15:51:51Z
dc.date.issued 2002
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/83168
dc.description.abstract In this paper, we discuss some problems concerning the formation of Uranus and Neptune. We find that the adoption of reduced Hill spheres as the region of close interaction between planetesimals introduces an enhancement of the gravitational cross-sections in previous numerical simulations. We also discuss a way to make possible the formation of Uranus and Neptune on time-scales shorter than the age of the Solar system. en
dc.format.extent 184-186 es
dc.language en es
dc.subject Accretion, accretion discs es
dc.subject Planets and satellites: formation es
dc.subject Planets and satellites: individual: Neptune es
dc.subject Planets and satellites: individual: Uranus es
dc.subject Solar system: formation es
dc.title On the accretion of Uranus and Neptune en
dc.type Articulo es
sedici.identifier.other doi:10.1046/j.1365-8711.2002.05104.x es
sedici.identifier.other eid:2-s2.0-0011736955 es
sedici.identifier.issn 0035-8711 es
sedici.creator.person Brunini, Adrián es
sedici.creator.person Melita, Mario Daniel es
sedici.subject.materias Ciencias Astronómicas es
sedici.description.fulltext true es
mods.originInfo.place Facultad de Ciencias Astronómicas y Geofísicas es
sedici.subtype Articulo es
sedici.rights.license Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
sedici.rights.uri http://creativecommons.org/licenses/by-nc-sa/4.0/
sedici.description.peerReview peer-review es
sedici.relation.journalTitle Monthly Notices of the Royal Astronomical Society es
sedici.relation.journalVolumeAndIssue vol. 330, no. 1 es


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Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) Except where otherwise noted, this item's license is described as Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)