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- W2008420439 abstract "As a simple model of a “star” one may take a rotating, self-gravitating fluid mass with a barotropic equation of state: p = P(p); the total mass M and a distribution of angular momentum per unit mass j are prescribed parameters. The existence of configurations (that is, density functions p(x), x E R3) satisfying the conditions of hydrodynamical equilibrium depends crucially upon the nature of the function P. When the condition" @default.
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- W2008420439 date "1981-12-01" @default.
- W2008420439 modified "2023-09-25" @default.
- W2008420439 title "Existence and dimensions of a rotating white dwarf" @default.
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- W2008420439 doi "https://doi.org/10.1016/0022-0396(81)90114-5" @default.
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