Structure-distortion of polytropic stars by differential rotation: Third- order perturbation theory

DOI10.1007/BF00642085zbMath0463.76095OpenAlexW2087532249MaRDI QIDQ1153819

G. A. Antonacopoulos, V. S. Geroyannis

Publication date: 1981

Published in: Astrophysics and Space Science (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1007/bf00642085

zbMATH Keywords

third-order perturbation theoryChandrasekhar's perturbation theoryrotating gaseous polytropestructure-distortion

Mathematics Subject Classification ID

General theory of rotating fluids (76U05) Applications to the sciences (65Z05) Galactic and stellar dynamics (85A05)

Related Items (3)

Rotating visco-polytropic models: Dissipative effects under the influence of a toroidal magnetic field ⋮ Chandrasekhar's perturbation method-oriented theories up to third order for uniformly and differentially-rotating polytropic stars: error- removing techniques ⋮ Numerical simulators of stability in astrophysical problems

Cites Work

• A second-order perturbation theory for differentially rotating gaseous polytropes
• Unnamed Item

This page was built for publication: Structure-distortion of polytropic stars by differential rotation: Third- order perturbation theory