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hal.structure.identifiersSE 2011
dc.contributor.authorCOSSOU, C.
hal.structure.identifierFORMATION STELLAIRE 2011
dc.contributor.authorPIERENS, A.
hal.structure.identifiersSE 2011
dc.contributor.authorRAYMOND, Sean N.
dc.date.issued2011-10
dc.date.conference2011
dc.description.abstractEnEarth- to Neptune-mass planets launch spiral density waves in gaseous protoplanetary disks and undergo type 1 migration. In isothermal disks, type 1 migration is inward and the migration timescale is inversely proportional to the planet mass. In radiative disks migration can be directed inward or outward, depending on the planet's mass and the disk's physical properties. For a given planet mass, there exist locations within the disk where the migration is convergent. We present results of hydrodynamic simulations of systems of planetary embryos of a few Earth masses embedded in radiative disks. We concentrate on the collective behavior of the system of embryos and their collisional growth.
dc.language.isoen
dc.source.titleEPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. p.509, 2011
dc.title.enMigration and growth of planetary embryos in radiative protoplanetary disks
dc.typeCommunication dans un congrès
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Planétologie et astrophysique de la terre [astro-ph.EP]
dc.subject.halPhysique [physics]/Astrophysique [astro-ph]/Planétologie et astrophysique de la terre [astro-ph.EP]
bordeaux.page509
bordeaux.countryFR
bordeaux.title.proceedingEPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. p.509, 2011
bordeaux.conference.cityNantes
bordeaux.peerReviewedoui
hal.identifierhal-00665146
hal.version1
hal.invitednon
hal.proceedingsoui
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-00665146v1
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