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dc.contributor.authorMOÓR, Attila
hal.structure.identifierLaboratoire d'études spatiales et d'instrumentation en astrophysique [LESIA (UMR_8109)]
dc.contributor.authorKRAL, Quentin
dc.contributor.authorÁBRAHÁM, Péter
dc.contributor.authorKÓSPÁL, Ágnes
hal.structure.identifierAMOR 2019
dc.contributor.authorDUTREY, Anne
hal.structure.identifierAMOR 2019
dc.contributor.authorDI FOLCO, E.
dc.contributor.authorHUGHES, A. Meredith
dc.contributor.authorJUHÁSZ, Attila
dc.contributor.authorPASCUCCI, Ilaria
hal.structure.identifierMax-Planck-Institut für Astronomie [MPIA]
dc.contributor.authorPAWELLEK, Nicole
dc.date.issued2019
dc.identifier.issn0004-637X
dc.description.abstractEnPrevious observations revealed the existence of CO gas at nearly protoplanetary level in several dust-rich debris disks around young A-type stars. Here we used the ALMA 7m-array to measure $^{13}$CO and C$^{18}$O emission toward two debris disks, 49 Cet and HD 32297, and detected similarly high CO content ($>$0.01M$_\oplus$). These high CO masses imply a highly efficient shielding of CO molecules against stellar and interstellar ultraviolet photons. Adapting a recent secondary gas disk model that considers both shielding by carbon atoms and self-shielding of CO, we can explain the observed CO level in both systems. Based on the derived gas densities we suggest that, in the HD 32297 disk, dust and gas are coupled and the dynamics of small grains is affected by the gaseous component. For 49 Cet, the question of coupling remains undecided. We found that the main stellar and disk propertiesof 49 Cet and HD 32297 are very similar to those of previously identified debris disks with high CO content. These objects constitute together the first known representatives of shielded debris disks.
dc.language.isoen
dc.publisherAmerican Astronomical Society
dc.subject.enAstrophysics - Earth and Planetary Astrophysics
dc.title.enNew millimeter CO observations of the gas-rich debris disks 49 Cet and HD 32297
dc.typeArticle de revue
dc.identifier.doi10.3847/1538-4357/ab4272
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Cosmologie et astrophysique extra-galactique [astro-ph.CO]
dc.identifier.arxiv1908.09685
bordeaux.journalThe Astrophysical Journal
bordeaux.pageid. 108
bordeaux.volume884
bordeaux.issue2
bordeaux.peerReviewedoui
hal.identifierhal-02282437
hal.version1
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-02282437v1
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