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dc.date.accessioned 2019-10-03T16:25:15Z
dc.date.available 2019-10-03T16:25:15Z
dc.date.issued 2010
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/82626
dc.description.abstract We investigate the motion of a two-planet coplanar system under the combined effects of mutual interaction and tidal dissipation. The secular behavior of the system is analyzed using two different approaches, restricting to the case of a more massive outer planet. First, we solve the exact equations of motion through the numerical simulation of the system evolution. We also compute the stationary solutions of the mean equations of motion based on a Hamiltonian formalism. An application to the real system CoRoT-7 is investigated. en
dc.format.extent 508-510 es
dc.language en es
dc.subject Celestial mechanics es
dc.title Tidal evolution of a close-in planet with a more massive outer companion en
dc.type Articulo es
sedici.identifier.other eid:2-s2.0-84882967233 es
sedici.identifier.other doi:10.1017/S1743921311021004 es
sedici.identifier.issn 1743-9213 es
sedici.creator.person Rodríguez, Adrian es
sedici.creator.person Ferraz Mello, Sylvio es
sedici.creator.person Michtchenko, Tatiana A. es
sedici.creator.person Beaugé, Cristian es
sedici.creator.person Miloni, Octavio es
sedici.subject.materias Ciencias Astronómicas es
sedici.description.fulltext true es
mods.originInfo.place Facultad de Ciencias Astronómicas y Geofísicas es
sedici.subtype Comunicacion 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.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-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) Excepto donde se diga explícitamente, este item se publica bajo la siguiente licencia Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)