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dc.contributor.authorKraus, S
dc.contributor.authorKreplin, A
dc.contributor.authorYoung, AK
dc.contributor.authorBate, MR
dc.contributor.authorMonnier, JD
dc.contributor.authorHarries, TJ
dc.contributor.authorAvenhaus, H
dc.contributor.authorKluska, J
dc.contributor.authorLaws, ASE
dc.contributor.authorRich, EA
dc.contributor.authorWillson, M
dc.contributor.authorAarnio, AN
dc.contributor.authorAdams, FC
dc.contributor.authorAndrews, SM
dc.contributor.authorAnugu, N
dc.contributor.authorBae, J
dc.contributor.authorten Brummelaar, T
dc.contributor.authorCalvet, N
dc.contributor.authorCure, M
dc.contributor.authorDavies, CL
dc.contributor.authorEnnis, J
dc.contributor.authorEspaillat, C
dc.contributor.authorGardner, T
dc.contributor.authorHartmann, L
dc.contributor.authorHinkley, S
dc.contributor.authorLabdon, A
dc.contributor.authorLanthermann, C
dc.contributor.authorLeBouquin, J-B
dc.contributor.authorSchaefer, GH
dc.contributor.authorSetterholm, BR
dc.contributor.authorWilner, D
dc.contributor.authorZhu, Z
dc.date.accessioned2020-08-04T14:56:16Z
dc.date.issued2020-09-04
dc.description.abstractYoung stars are surrounded by a circumstellar disk of gas and dust, within which planet formation can occur. Gravitational forces in multiple star systems can disrupt the disk. Theoretical models predict that if the disk is misaligned with the orbital plane of the stars, the disk should warp and break into precessing rings, a phenomenon known as disk tearing. We present observations of the triple star system GW Orionis, finding evidence for disk tearing. Our images show an eccentric ring that is misaligned with the orbital planes and the outer disk. The ring casts shadows on a strongly warped intermediate region of the disk. If planets can form within the warped disk, disk tearing could provide a mechanism for forming wide-separation planets on oblique orbitsen_GB
dc.description.sponsorshipEuropean Union Horizon 2020en_GB
dc.description.sponsorshipEuropean Union FP7en_GB
dc.description.sponsorshipScience and Technology Facilities Council (STFC)en_GB
dc.description.sponsorshipNSFen_GB
dc.description.sponsorshipNASAen_GB
dc.description.sponsorshipKU Leuvenen_GB
dc.identifier.citationVol. 369 (6508), pp. 1233-1238en_GB
dc.identifier.doi10.1126/science.aba4633
dc.identifier.grantnumber639889en_GB
dc.identifier.grantnumber681601en_GB
dc.identifier.grantnumber339248en_GB
dc.identifier.grantnumber1918673en_GB
dc.identifier.grantnumberNSFAST1506540en_GB
dc.identifier.grantnumberNSF-AST 1830728en_GB
dc.identifier.grantnumberNNX16AD43Gen_GB
dc.identifier.grantnumberC14/17/082en_GB
dc.identifier.grantnumberHST-HF2-51427.001-Aen_GB
dc.identifier.urihttp://hdl.handle.net/10871/122315
dc.language.isoenen_GB
dc.publisherAmerican Association for the Advancement of Science (AAAS)en_GB
dc.rightsCopyright © 2020 The Authors, some rights reserved; exclusive licensee American Association for the Advancement of Science.
dc.titleA triple star system with a misaligned and warped circumstellar disk shaped by disk tearingen_GB
dc.typeArticleen_GB
dc.date.available2020-08-04T14:56:16Z
dc.descriptionThis is the author accepted manuscript. The final version is available from AAAS via the DOI in this record.en_GB
dc.identifier.eissn1095-9203
dc.identifier.journalScienceen_GB
dc.rights.urihttp://www.rioxx.net/licenses/all-rights-reserveden_GB
dcterms.dateAccepted2020-07-24
exeter.funder::European Commissionen_GB
exeter.funder::Science and Technology Facilities Councilen_GB
rioxxterms.versionAMen_GB
rioxxterms.licenseref.startdate2020-07-24
rioxxterms.typeJournal Article/Reviewen_GB
refterms.dateFCD2020-08-04T14:04:22Z
refterms.versionFCDAM
refterms.dateFOA2020-09-04T12:31:49Z
refterms.panelBen_GB


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