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dc.contributor.authorVAN BOEKEL, Roy
dc.contributor.authorABRAHAM, Peter
dc.contributor.authorCORREIA, Serge
dc.contributor.authorDE KOTER, Alex
dc.contributor.authorDOMINIK, Carsten
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.contributor.authorHENNING, Thomas
dc.contributor.authorKOSPAL, Agnes
dc.contributor.authorLACHAUME, Regis
dc.contributor.authorLEINERT, Christoph
dc.contributor.authorLINZ, Hendrik
dc.contributor.authorMIN, Michiel
dc.contributor.authorMOSONI, Laszlo
dc.contributor.authorPREIBISCH, Thomas
dc.contributor.authorQUANZ, Sascha
dc.contributor.authorRATZKA, Thorsten
dc.contributor.authorSCHEGERER, Alexander
dc.contributor.authorWATERS, Rens
dc.contributor.authorWOLF, Sebastian
dc.contributor.authorZINNECKER, Hans
dc.date.created2006
dc.date.issued2006
dc.date.conference2006
dc.description.abstractEnWe report on observations of circumstellar disks around young stars that have been obtained with the MIDI instrument, which is mounted on the VLT Interferometer and operates in the 10 micrometer atmospheric window. The maximum spatial resolution of 5 milli-arcsec corresponds to sub-AU scales at the distance to nearby star formation regions. Thus, we can study the disks on the spatial scales at which important processes occur, such as accretion, dust processing, and planet formation. The main results obtained so far can be summarized as follows: 1. The measured interferometric visibilities are in good qualitative agreement with those predicted by models of circumstellar disks. In particular, a predicted correlation between the strength of the far-infrared excess and the spatial structure of the disk is confirmed by direct measurements; 2. In several objects strong evidence for deviations from circular symmetry is present, indicating that an inclined disk is indeed the dominant component seen in the mid-infrared; 3. The dust properties are not uniform over the disk, but are instead a strong function of distance to the central star. The dust in the innermost disk regions is observed to be more ``processed'' than the dust further out, both in Herbig Ae star disks and in those around T-Tauri stars.
dc.language.isoen
dc.publisherEdited by Monnier, John D.; Schöller, Markus; Danchi, William C.
dc.source.title2006SPIE.6268E..13V - Advances in Stellar Interferometry. Proceedings of the SPIE,
dc.subject.encircumstellar
dc.subject.endisk
dc.subject.endust
dc.subject.enevolution
dc.subject.eninfrared
dc.subject.eninterferometry
dc.subject.enplanet formation
dc.subject.enradiative transfer
dc.subject.enstar formation
dc.subject.enYSO
dc.title.enDisks around young stars with VLTI/MIDI
dc.typeCommunication dans un congrès
dc.identifier.doi10.1117/12.673777
dc.subject.halPhysique [physics]/Astrophysique [astro-ph]/Cosmologie et astrophysique extra-galactique [astro-ph.CO]
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]
dc.identifier.arxivastro-ph/0607387
bordeaux.page62680D (2006)
bordeaux.volume6268
bordeaux.countryFR
bordeaux.title.proceeding2006SPIE.6268E..13V - Advances in Stellar Interferometry. Proceedings of the SPIE,
bordeaux.peerReviewedoui
hal.identifierhal-00128310
hal.version1
hal.invitednon
hal.proceedingsoui
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-00128310v1
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