The dynamics of the radiative envelope of rapidly rotating stars

DOI10.1051/0004-6361:20054433zbMath1096.85009arXivastro-ph/0602040OpenAlexW3103964835WikidataQ68592713 ScholiaQ68592713MaRDI QIDQ5480233

Michel Rieutord

Publication date: 27 July 2006

Published in: Astronomy & Astrophysics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/astro-ph/0602040

zbMATH Keywords

hydrodynamicsstars: rotation

Mathematics Subject Classification ID

Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Galactic and stellar structure (85A15)

Related Items (5)

Baroclinically-driven flows and dynamo action in rotating spherical fluid shells ⋮ Stress-driven spin-down of a viscous fluid within a spherical shell ⋮ Inertial waves in a differentially rotating spherical shell ⋮ An algorithm for computing the 2D structure of fast rotating stars ⋮ Gravito-inertial waves in a differentially rotating spherical shell

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