Use of Roche coordinates in the problems of small oscillations of tidally distorted stellar models

DOI10.1007/BF00643465zbMath0381.70022OpenAlexW2045460933MaRDI QIDQ1248346

K. Appert

Publication date: 1978

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

Full work available at URL: https://doi.org/10.1007/bf00643465

Mathematics Subject Classification ID

Stability for problems in linear vibration theory (70J25) Modal analysis in linear vibration theory (70J10) Galactic and stellar dynamics (85A05)

Related Items (4)

Effect of Coriolis force on the shapes of rotating stars and stars in binary systems ⋮ Effect of Coriolis force on the equilibrium structures of rotating stars and stars in binary systems ⋮ Use of Roche coordinates in the problems of small oscillations of tidally-distorted stellar models. II. Effects of second-order terms in tidal distortion ⋮ Effect of rotational and tidal distortions on the periods of small adiabatic oscillations of stellar models

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