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dc.contributor.authorLIN, Min-Kai
hal.structure.identifierECLIPSE 2018
dc.contributor.authorPIERENS, A.
dc.date.issued2018-04-18
dc.identifier.issn0035-8711
dc.description.abstractEnLarge-scale, dust-trapping vortices may account for observations of asymmetric protoplanetary discs. Disc vortices are also potential sites for accelerated planetesimal formation by concentrating dust grains. However, in 3D discs vortices are subject to destructive `elliptic instabilities', which reduces their viability as dust traps. The survival of vortices in 3D accretion discs is thus an important issue to address. In this work, we perform shearing box simulations to show that disc self-gravity enhances the survival of 3D vortices, even when self-gravity is weak in the classic sense (e.g. with a Toomre Q ≃ 5). We find a 3D self-gravitating vortex can grow on secular time-scales in spite of the elliptic instability. The vortex aspect ratio decreases as it strengthens, which feeds the elliptic instability. The result is a 3D vortex with a turbulent core that persists for ˜103 orbits. We find when gravitational and hydrodynamic stresses become comparable, the vortex may undergo episodic bursts, which we interpret as an interaction between elliptic and gravitational instabilities. We estimate the distribution of dust particles in self-gravitating, turbulent vortices. Our results suggest large-scale vortices in protoplanetary discs are more easily observed at large radii.
dc.language.isoen
dc.publisherOxford University Press (OUP): Policy P - Oxford Open Option A
dc.typeArticle de revue
dc.identifier.doi10.1093/mnras/sty947
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Planétologie et astrophysique de la terre [astro-ph.EP]
dc.identifier.arxiv1805.05825
bordeaux.journalMonthly Notices of the Royal Astronomical Society
bordeaux.page575-591
bordeaux.volume478
bordeaux.issue1
bordeaux.peerReviewedoui
hal.identifierhal-01777647
hal.version1
hal.popularnon
hal.audienceInternationale
dc.title.itVortex survival in 3D self-gravitating accretion discs
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-01777647v1
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