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- W3150578726 abstract "In this paper, it is proved by using the method in [1] that the stability criteria of rotat-ing liquid stars, which depend on all of the normal modes of oscillation, are consistent with itssecular stability criteria, if liquid stars are assumed to consist of incompressible, self-gravi-tating masses of viscous liquid. Moreover, the experimental evidence of the conclusion isprovided by the Columbus problem. This conclusion was predicted without proof byThomson and Tait in 1883. Thus,it is reaffirmed that the evolution process of the rotatingliquid stars in quasi-stationary state should be judged by the secular stability criteria. Jeans-Darwin's fission theory of binary stars, which has been denied during the last three decades,ought to be evaluated anew." @default.
- W3150578726 created "2021-04-13" @default.
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- W3150578726 date "1981-01-20" @default.
- W3150578726 modified "2023-09-24" @default.
- W3150578726 title "ON THE STABILITY OF ROTATING LIQUID STARS" @default.
- W3150578726 doi "https://doi.org/10.1360/ya1981-24-1-61" @default.
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