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dc.date.accessioned 2019-10-03T15:17:59Z
dc.date.available 2019-10-03T15:17:59Z
dc.date.issued 2011-11
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/82616
dc.description.abstract We calculate the simultaneous in situ formation of Jupiter and Saturn by the core instability mechanism considering the oligarchic growth regime for the accretion of planetesimals. We consider a density distribution for the size of planetesimals and planetesimals migration. The planets are immersed in a realistic protoplanetary disk that evolves with time. We find that, within the classical model of solar nebula, the isolated formation of Jupiter and Saturn undergoes significant change when it occurs simultaneously. en
dc.format.extent 428-429 es
dc.language en es
dc.subject Planets and satellites: formation es
dc.subject Jupiter es
dc.subject Saturn es
dc.title Simultaneous formation of Jupiter and Saturn en
dc.type Articulo es
sedici.identifier.other http://dx.doi.org/10.1017/s1743921311020655 es
sedici.identifier.issn 1743-9213 es
sedici.creator.person Guilera, Octavio Miguel es
sedici.creator.person Brunini, Adrián es
sedici.creator.person Benvenuto, Omar Gustavo es
sedici.subject.materias Ciencias Astronómicas es
sedici.description.fulltext true es
mods.originInfo.place Facultad de Ciencias Astronómicas y Geofísicas es
mods.originInfo.place Instituto de Astrofísica de La Plata es
sedici.subtype Comunicacion es
sedici.rights.license Creative Commons Attribution 4.0 International (CC BY 4.0)
sedici.rights.uri http://creativecommons.org/licenses/by/4.0/
sedici.relation.event IAU Symposium 276 (Torino, Italy, 2010) es
sedici.description.peerReview peer-review es
sedici.relation.journalTitle Proceedings of the International Astronomical Union es
sedici.relation.journalVolumeAndIssue vol. 6, no. S276 es


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