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hal.structure.identifierLaboratoire d'Astrophysique de Grenoble [LAOG]
dc.contributor.authorBEUST, H.
hal.structure.identifierLaboratoire d'astrodynamique, d'astrophysique et d'aéronomie de bordeaux [L3AB]
hal.structure.identifierObservatoire aquitain des sciences de l'univers [OASU]
hal.structure.identifierLaboratoire d'Astrophysique de Bordeaux [Pessac] [LAB]
dc.contributor.authorDUTREY, Anne
dc.date.issued2005
dc.identifier.issn0004-6361
dc.description.abstractEnThe GG Tauri system is a prototype example of a young, pre-main sequence multiple stellar system. Both millimeter and optical observations reveal that the central binary (GG Tau A) harbors a ring-shape circumbinary disk. In this paper, we analyse a compilation of astrometric data of the GG Tau A binary over 12 years that allow us, in combination with information coming from the disk observations (millimeter data), to derive a fairly accurate fit of the orbit (a=32.4 AU, e=0.34). We also perform a dynamical study of the circumbinary disk, and show that in order to be in agreement with the orbit deduced from the fit, the inner gap of the disk should be approximatively twice as small as observed. We show that if we allow the error bars on the astrometric data to be larger, another orbit may be found (a=62 AU, e=0.35), compatible with the location of the inner disk gap, although only marginally compatible with the astrometric data. Possible solutions to solve this discrepancy are discussed.
dc.language.isoen
dc.publisherEDP Sciences
dc.subject.enplanetary systems: protoplanetary disks
dc.subject.enstars: individual: GG Tau
dc.subject.enmethods: numerical
dc.subject.encelestial mechanics
dc.subject.enstars: circumstellar matter
dc.title.enDynamics of the young multiple system GG Tauri.
dc.title.enI. Orbital fits and inner edge of the circumbinary disk of GG Tau A
dc.typeArticle de revue
dc.identifier.doi10.1051/0004-6361:20042441
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Astrophysique galactique [astro-ph.GA]
bordeaux.journalAstronomy and Astrophysics - A&A
bordeaux.page585-594
bordeaux.volume439
bordeaux.issue2
bordeaux.peerReviewedoui
hal.identifierhal-00417586
hal.version1
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-00417586v1
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