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dc.date.accessioned 2010-10-05T13:29:15Z
dc.date.available 2010-10-05T03:00:00Z
dc.date.issued 2009
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/2090
dc.description.abstract Aims. The equation of state calculated by Saumon and collaborators has been adopted in most core-accretion simulations of giant-planet formation performed to date. Since some minor errors have been found in their original paper, we present revised simulations of giant-planet formation that considers a corrected equation of state. Methods. We employ the same code as Fortier and collaborators in repeating our previous simulations of the formation of Jupiter. Results. Although the general conclusions of Fortier and collaborators remain valid, we obtain significantly lower core masses and shorter formation times in all cases considered. Conclusions. The minor errors in the previously published equation of state have been shown to affect directly the adiabatic gradient and the specific heat, causing an overestimation of both the core masses and formation times. en
dc.format.extent 1249-1252 es
dc.language en es
dc.subject planetología es
dc.subject acreción es
dc.title Oligarchic planetesimal accretion and giant planet formation II en
dc.type Articulo es
sedici.identifier.uri http://www.aanda.org/index.php?option=com_article&access=standard&Itemid=129&url=/articles/aa/full_html/2009/24/aa11367-08/aa11367-08.html es
sedici.identifier.other https://doi.org/10.1051/0004-6361/200811367
sedici.identifier.issn 1432-0746 es
sedici.creator.person Fortier, Andrea es
sedici.creator.person Benvenuto, Omar Gustavo es
sedici.creator.person Brunini, Adrián es
sedici.subject.materias Ciencias Astronómicas es
sedici.description.fulltext true es
mods.originInfo.place Grupo de Ciencias Planetarias es
sedici.subtype Comunicacion es
sedici.rights.license Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International (CC BY-NC-ND 4.0)
sedici.rights.uri http://creativecommons.org/licenses/by-nc-nd/4.0/
sedici.description.peerReview peer-review es
sedici2003.identifier ARG-UNLP-ART-0000006635 es
sedici.relation.journalTitle Astronomy and Astrophysics es
sedici.relation.journalVolumeAndIssue vol. 500, no. 3 es


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