摘要: The aim of the present paper will be to detail explicit form equations which govern first-order oscillations fast-rotating globes self-gravitating fluids; with due account taken effects arising from centrifugal as well Coriolis force. As such configurations oscillate in general about distorted figures equilibrium, governing them can conveniently expressed terms Clairaut coordinates, associated spheroidal figures, and introduced our previous (Kopal, 1980) for this purpose.
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