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hal.structure.identifierAMOR 2016
dc.contributor.authorDUTREY, Anne
hal.structure.identifierAMOR 2016
dc.contributor.authorDI FOLCO, E.
hal.structure.identifierSpace Telescope Science Institute [STSci]
dc.contributor.authorBECK, Tracy
hal.structure.identifierAMOR 2016
dc.contributor.authorGUILLOTEAU, S.
dc.date.issued2016-12
dc.identifier.issn0935-4956
dc.description.abstractEnIn binary stellar systems, exoplanet searches have revealed planetary mass companions orbiting both in circumstellar and in circumbinary orbits. Modelling studies suggest increased dynamical complexity around the young stars that form such systems. Circumstellar and circumbinary disks likely exhibit different physical conditions for planet formation, which also depends on the stellar separation. Although binaries and higher order multiple stars are relatively common in nearby star-forming regions, surprisingly few systems with circumbinary distributions of proto-planetary material have been found. With its spectacular ring of dust and gas encircling the central triple star, one such system, GG Tau A, has become a unique laboratory for investigating the physics of circumsystem gas and dust evolution. We review here its physical properties.
dc.language.isoen
dc.publisherSpringer Verlag
dc.title.enGG Tau: the ringworld and beyond. Mass accretion and planetary formation in young multiple stellar systems
dc.typeArticle de revue
dc.identifier.doi10.1007/s00159-015-0091-5
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Cosmologie et astrophysique extra-galactique [astro-ph.CO]
bordeaux.journalAstronomy and Astrophysics Review
bordeaux.pageid. #5
bordeaux.volume24
bordeaux.peerReviewedoui
hal.identifierhal-01278262
hal.version1
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-01278262v1
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