BOUTIN-BASILLAIS, B.; HURÉ, J.-M.

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Licencia de uso del documento

BOUTIN-BASILLAIS, B.
ECLIPSE 2018

HURÉ, J.-M.
ECLIPSE 2018

Idioma

Communication dans un congrès

Este ítem está publicado en

2018-07-03, Bordeaux. 2018

Resumen en inglés

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.< Leer menos

Palabras clave en inglés

Methods: numerical

Stars: rotation

Equation of state

Gravitation

Orígen

Importado de Hal

Centros de investigación

Laboratoire d'Astrophysique de Bordeaux (LAB) - UMR 5804