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Physical and chemical structure of planet-forming disks probed by millimeter observations and modeling

hal.structure.identifierAMOR 2014
dc.contributor.authorDUTREY, Anne
hal.structure.identifierA.N. Severtsov Institute of Ecology and Evolution
dc.contributor.authorSEMENOV, Dmitry
hal.structure.identifierAMOR 2014
hal.structure.identifierInstitut de RadioAstronomie Millimétrique [IRAM]
dc.contributor.authorCHAPILLON, E.
dc.contributor.authorGORTI, Uma
hal.structure.identifierAMOR 2014
dc.contributor.authorGUILLOTEAU, S.
hal.structure.identifierFORMATION STELLAIRE 2014
dc.contributor.authorHERSANT, F.
dc.contributor.authorHOGERHEIJDE, Michiel
dc.contributor.authorHUGHES, Meredith
hal.structure.identifierLeibniz-Institut für Astrophysik Potsdam [AIP]
dc.contributor.authorMEEUS, Gwendolyn
dc.contributor.authorNOMURA, Hideko
hal.structure.identifierInstitut de RadioAstronomie Millimétrique [IRAM]
hal.structure.identifierInstitut de Planétologie et d'Astrophysique de Grenoble [IPAG ]
dc.contributor.authorPIÉTU, Vincent
dc.contributor.authorQI, Chunhua
hal.structure.identifierAMOR 2014
dc.contributor.authorWAKELAM, Valentine
dc.date.created2014-02-14
dc.date.issued2014
dc.date.conference2013-07-15
dc.description.abstractEnProtoplanetary disks composed of dust and gas are ubiquitous around young stars and are commonly recognized as nurseries of planetary systems. Their lifetime, appearance, and structure are determined by an interplay between stellar radiation, gravity, thermal pressure, magnetic field, gas viscosity, turbulence, and rotation. Molecules and dust serve as major heating and cooling agents in disks. Dust grains dominate the disk opacities, reprocess most of the stellar radiation, and shield molecules from ionizing UV/X-ray photons. Disks also dynamically evolve by building up planetary systems which drastically change their gas and dust density structures. Over the past decade significant progress has been achieved in our understanding of disk chemical composition thanks to the upgrade or advent of new millimeter/Infrared facilities (SMA, PdBI, CARMA, Herschel, e-VLA, ALMA). Some major breakthroughs in our comprehension of the disk physics and chemistry have been done since PPV. This review will present and discuss the impact of such improvements on our understanding of the disk physical structure and chemical composition.
dc.language.isoen
dc.title.enPhysical and chemical structure of planet-forming disks probed by millimeter observations and modeling
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]/Physique [physics]/Physique de l'espace [physics.space-ph]
dc.subject.halPhysique [physics]/Astrophysique [astro-ph]/Astrophysique stellaire et solaire [astro-ph.SR]
dc.subject.halPhysique [physics]/Astrophysique [astro-ph]/Cosmologie et astrophysique extra-galactique [astro-ph.CO]
dc.identifier.arxiv1402.3503
bordeaux.page317-338
bordeaux.conference.titleProtostars and Planets VI, Henrik Beuther, Ralf S. Klessen, Cornelis P. Dullemond, and Thomas Henning (eds.), University of Arizona Press, Tucson, 914 pp., p.317-338
bordeaux.countryDE
bordeaux.conference.cityHeidelberg
bordeaux.peerReviewedoui
hal.identifierhal-00949240
hal.version1
hal.invitednon
hal.proceedingsoui
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-00949240v1
bordeaux.COinSctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.date=2014&rft.spage=317-338&rft.epage=317-338&rft.au=DUTREY,%20Anne&SEMENOV,%20Dmitry&CHAPILLON,%20E.&GORTI,%20Uma&GUILLOTEAU,%20S.&rft.genre=unknown


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