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Article: Modeling the resonant planetary system GJ 876

TitleModeling the resonant planetary system GJ 876
Authors
Kley, WLee, MHMurray, NPeale, SJ
KeywordsAccretion, Accretion Disks
Planets And Satellites: Formation Hydrodynamics Methods: N-Body Simulations
Issue Date2005
PublisherE D P Sciences. The Journal's web site is located at http://www.aanda.org
Citation
Astronomy And Astrophysics, 2005, v. 437 n. 2, p. 727-742 How to Cite?
DOI: http://dx.doi.org/10.1051/0004-6361:20052656
AbstractThe evolution of the GJ 876 system using two-dimensional hydrodynamical simulations including viscous heating and radiative cooling was discussed. It was found that the relaxed disk remained circular in all models for low planet-to-star mass ratio q2, but becomes eccentric for high mass ratios for those models with fixed temperature structure. A more comprehensive set of numerical calculations treating the evolution of two planets interacting with their protoplanetary disk was presented with special emphasis on the resonant system GJ 876. The results show that it was possible to reduce the final values of the eccentricities close to the observed values.
Persistent Identifierhttp://hdl.handle.net/10722/151155
ISSN
0004-6361
2021 Impact Factor: 6.240
2020 SCImago Journal Rankings: 2.137
ISI Accession Number ID
WOS:000229978400037
References
References in Scopus

 

DC FieldValueLanguage
dc.contributor.authorKley, Wen_US
dc.contributor.authorLee, MHen_US
dc.contributor.authorMurray, Nen_US
dc.contributor.authorPeale, SJen_US
dc.date.accessioned2012-06-26T06:17:44Z-
dc.date.available2012-06-26T06:17:44Z-
dc.date.issued2005en_US
dc.identifier.citationAstronomy And Astrophysics, 2005, v. 437 n. 2, p. 727-742en_US
dc.identifier.issn0004-6361en_US
dc.identifier.urihttp://hdl.handle.net/10722/151155-
dc.description.abstractThe evolution of the GJ 876 system using two-dimensional hydrodynamical simulations including viscous heating and radiative cooling was discussed. It was found that the relaxed disk remained circular in all models for low planet-to-star mass ratio q2, but becomes eccentric for high mass ratios for those models with fixed temperature structure. A more comprehensive set of numerical calculations treating the evolution of two planets interacting with their protoplanetary disk was presented with special emphasis on the resonant system GJ 876. The results show that it was possible to reduce the final values of the eccentricities close to the observed values.en_US
dc.languageengen_US
dc.publisherE D P Sciences. The Journal's web site is located at http://www.aanda.orgen_US
dc.relation.ispartofAstronomy and Astrophysicsen_US
dc.subjectAccretion, Accretion Disksen_US
dc.subjectPlanets And Satellites: Formation Hydrodynamics Methods: N-Body Simulationsen_US
dc.titleModeling the resonant planetary system GJ 876en_US
dc.typeArticleen_US
dc.identifier.emailLee, MH:mhlee@hku.hken_US
dc.identifier.authorityLee, MH=rp00724en_US
dc.description.naturelink_to_subscribed_fulltexten_US
dc.identifier.doi10.1051/0004-6361:20052656en_US
dc.identifier.scopuseid_2-s2.0-21644457105en_US
dc.relation.referenceshttp://www.scopus.com/mlt/select.url?eid=2-s2.0-21644457105&selection=ref&src=s&origin=recordpageen_US
dc.identifier.volume437en_US
dc.identifier.issue2en_US
dc.identifier.spage727en_US
dc.identifier.epage742en_US
dc.identifier.isiWOS:000229978400037-
dc.publisher.placeFranceen_US
dc.identifier.scopusauthoridKley, W=7004830216en_US
dc.identifier.scopusauthoridLee, MH=7409119699en_US
dc.identifier.scopusauthoridMurray, N=7201513155en_US
dc.identifier.scopusauthoridPeale, SJ=6602697819en_US
dc.identifier.citeulike6566905-
dc.identifier.issnl0004-6361-

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