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hal.structure.identifieraMOR 2011
dc.contributor.authorDUTREY, Anne
dc.date.issued2011
dc.date.conference2011
dc.description.abstractEnTTauri disks located in nearby star-forming regions (e.g. Taurus-Auriga at 140 pc) are thought to be the site of planet formation, since proto-planetary disks orbiting around active (still accreting) TTauri stars should contain, in many cases, enough gas to form giant gaseous planets. As such, circumstellar disks are ideal laboratories to study planet formation, provided the gas and dust observations have enough sensitivity and resolving power. I will focus in these proceedings, on recent results of molecular observations which unveil the physical conditions of gas disks and reveal the weakness of our current understanding and modeling.
dc.language.isoen
dc.source.title2011IAUS..280..103D - The Molecular Universe, Proceedings of the International Astronomical Union, IAU Symposium, Volume 280, p. 103-113, 2011
dc.title.enMillimetre/Sub-millimetre Observations of Circumstellar Disks
dc.typeCommunication dans un congrès
dc.identifier.doi10.1017/S1743921311024902
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Cosmologie et astrophysique extra-galactique [astro-ph.CO]
dc.subject.halPhysique [physics]/Astrophysique [astro-ph]/Cosmologie et astrophysique extra-galactique [astro-ph.CO]
bordeaux.page103-113
bordeaux.volume280
bordeaux.countryES
bordeaux.title.proceeding2011IAUS..280..103D - The Molecular Universe, Proceedings of the International Astronomical Union, IAU Symposium, Volume 280, p. 103-113, 2011
bordeaux.conference.cityTolede
bordeaux.peerReviewedoui
hal.identifierhal-00665188
hal.version1
hal.invitedoui
hal.proceedingsoui
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-00665188v1
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