hal.structure.identifier	ECLIPSE 2018
dc.contributor.author	BOUTIN-BASILLAIS, B.
hal.structure.identifier	ECLIPSE 2018
dc.contributor.author	HURÉ, J.-M.
dc.date.issued	2018
dc.date.conference	2018-07-03
dc.description.abstractEn	We present an efficient multi-body code devoted to self-gravitating polytropic stars and rings in mutual gravitational interaction. The code implements the Self-Consistent Field method which captures solutions in an iterative manner. It works for any positive polytropic index, rotation law and configuration (axis ratios and relative separations). The number of bodies is free. We have investigated a wide range of equilibria involving 2 up to 8 bodies. A model for the disk around HL Tau is currently under progress.
dc.language.iso	en
dc.subject.en	Methods: numerical
dc.subject.en	Stars: rotation
dc.subject.en	Equation of state
dc.subject.en	Gravitation
dc.title.en	Multi-body figures of equilibrium in axial symmetry
dc.type	Communication dans un congrès
dc.subject.hal	Planète et Univers [physics]/Astrophysique [astro-ph]/Planétologie et astrophysique de la terre [astro-ph.EP]
bordeaux.country	FR
bordeaux.conference.city	Bordeaux
bordeaux.peerReviewed	oui
hal.identifier	hal-01981696
hal.version	1
hal.invited	non
hal.proceedings	non
hal.popular	non
hal.audience	Internationale
hal.origin.link	https://hal.archives-ouvertes.fr//hal-01981696v1
bordeaux.COinS	ctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.date=2018&rft.au=BOUTIN-BASILLAIS,%20B.&HUR%C3%89,%20J.-M.&rft.genre=unknown

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Multi-body figures of equilibrium in axial symmetry