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dc.date.accessioned 2010-10-05T16:08:05Z
dc.date.available 2010-10-05T03:00:00Z
dc.date.issued 2008
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/2093
dc.description.abstract With the aim of studying the final mass distribution of extrasolar planets, we have developed a simple model based on the core instability model, which allows us to form a large population of planets and make them evolve in circumstellar discs with various initial conditions. We investigate the consequences that different prescriptions for the solid and gas accretion rates would have on this distribution and found that it is strongly dependent on the adopted model for the gas accretion. en
dc.format.extent 463-468 es
dc.language en es
dc.subject planets and satellites es
dc.subject planetología es
dc.subject Sistema Solar es
dc.subject solar system: formation es
dc.subject astrofísica es
dc.title Core instability models of giant planet accretion and the planetary desert en
dc.type Articulo es
sedici.identifier.uri http://mnras.oxfordjournals.org/content/387/1/463 es
sedici.identifier.other https://doi.org/10.1111/j.1365-2966.2008.13261.x es
sedici.identifier.issn 1365-2966 es
sedici.creator.person Miguel, Yamila es
sedici.creator.person Brunini, Adrián 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-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-0000006638 es
sedici.relation.journalTitle Monthly Notices of the Royal Astronomical Society es
sedici.relation.journalVolumeAndIssue vol. 387, no. 1 es


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Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International (CC BY-NC-ND 4.0) Excepto donde se diga explícitamente, este item se publica bajo la siguiente licencia Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International (CC BY-NC-ND 4.0)