The possibility of non-synchronism of convective secondaries in close binary stars

DOI10.1093/MNRAS/204.2.433zbMath0578.76053OpenAlexW2075173602MaRDI QIDQ3701077

J. C. B. Papaloizou, Christopher Campbell

Publication date: 1983

Published in: Monthly Notices of the Royal Astronomical Society (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1093/mnras/204.2.433

zbMATH Keywords

synchronization rateturbulent viscositycataclysmic systemclose rotating binary systemlow mass convective secondarynon-synchronous velocity fieldweak tidal distortion

Mathematics Subject Classification ID

Hydrology, hydrography, oceanography (86A05) Three-body problems (70F07) Stability and instability of geophysical and astrophysical flows (76E20)

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