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Main Authors: Huré, Jean-Marc, Staelen, Clément
Format: Preprint
Published: 2024
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Online Access:https://arxiv.org/abs/2406.19210
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author Huré, Jean-Marc
Staelen, Clément
author_facet Huré, Jean-Marc
Staelen, Clément
contents We show that a rigidly rotating, homogeneous ellipsoid of revolution threaded by a uniform, coaxial magnetic field is a possible figure of equilibrium. While the spheroidal shape is fully preserved, the rotation rate is modified. Accordingly, we extend the fundamental formula by Maclaurin. In contrast with the non-magnetic case, prolate shapes are permitted, but there are critical states in the form of maximum elongations, depending on ionisation fraction, ion/electron drift, magnetic field and mass-density. As checked from numerical simulations based on the Self-Consistent-Field method, prolate states survive to gas compressibility. The relevance to interstellar clouds is outlined.
format Preprint
id arxiv_https___arxiv_org_abs_2406_19210
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle The Maclaurin spheroid in disguise. New figures of equilibrium with external magnetic support
Huré, Jean-Marc
Staelen, Clément
Astrophysics of Galaxies
We show that a rigidly rotating, homogeneous ellipsoid of revolution threaded by a uniform, coaxial magnetic field is a possible figure of equilibrium. While the spheroidal shape is fully preserved, the rotation rate is modified. Accordingly, we extend the fundamental formula by Maclaurin. In contrast with the non-magnetic case, prolate shapes are permitted, but there are critical states in the form of maximum elongations, depending on ionisation fraction, ion/electron drift, magnetic field and mass-density. As checked from numerical simulations based on the Self-Consistent-Field method, prolate states survive to gas compressibility. The relevance to interstellar clouds is outlined.
title The Maclaurin spheroid in disguise. New figures of equilibrium with external magnetic support
topic Astrophysics of Galaxies
url https://arxiv.org/abs/2406.19210