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

The possibility of non-synchronism of convective secondaries in close binary stars (Q3701077)

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The possibility of non-synchronism of convective secondaries in close binary stars
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    The possibility of non-synchronism of convective secondaries in close binary stars (English)
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    1983
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    weak tidal distortion
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    synchronization rate
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    cataclysmic system
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    close rotating binary system
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    non-synchronous velocity field
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    low mass convective secondary
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    turbulent viscosity
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