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hal.structure.identifierECLIPSE 2019
dc.contributor.authorBOUTIN-BASILLAIS, B.
hal.structure.identifierECLIPSE 2019
dc.contributor.authorHURÉ, J.-M.
dc.date.issued2019-06-19
dc.identifier.issn0035-8711
dc.description.abstractEnThe equilibrium of incompressible spheroid-ring systems in rigid rotation is investigated by numerical means for a unity density contrast. A great diversity of binary configurations is obtained, with no limit neither in the mass ratio, nor in the orbital separation. We found only detached binaries, meaning that the end-point of the ɛ2-sequence is the single binary state in strict contact, easily prone to mass-exchange. The solutions show a remarkable confinement in the rotation frequency-angular momentum diagram, with a total absence of equilibrium for Ω2/πGρ ≳ 0.21. A short band of degeneracy is present next to the one-ring sequence. We unveil a continuum of bifurcations all along the ascending side of the Maclaurin sequence for eccentricities of the ellipsoid less than ≈0.612 and which involves a gradually expanding, initially massless loop.
dc.language.isoen
dc.publisherOxford University Press (OUP): Policy P - Oxford Open Option A
dc.subject.enMethods: numerical
dc.subject.enGravitation
dc.subject.enstars: interiors
dc.subject.enstars: rotation
dc.subject.enMethods: analytical
dc.title.enRigidly rotating, incompressible spheroid-ring systems: new bifurcations, critical rotations and degenerate states
dc.typeArticle de revue
dc.identifier.doi10.1093/mnras/stz1615
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Planétologie et astrophysique de la terre [astro-ph.EP]
bordeaux.journalMonthly Notices of the Royal Astronomical Society
bordeaux.page4504-4509
bordeaux.volume487
bordeaux.issue4
bordeaux.peerReviewedoui
hal.identifierhal-02165831
hal.version1
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-02165831v1
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