[1] Chanillo S, Li Y Y. On diameters of uniformly rotating stars. Comm Math Phys, 1994, 166(2): 417–430
[2] Deng Y B, Liu T P, et al. Solutions of Euler-Possion equations for gaseous stars. Arch Ration Mech Anal, 2002, 164(3): 261–285
[3] Deng Y B, Xie H Z. Multiple stationary solutions of Euler-Poisson equations for non-isentropic gaseous stars. Acta Math Sci, 2010, 30B(6): 2077–2088
[4] Deng Y B, Yang T. Multiplicity of stationary solutions to the Euler-Poisson equations. J Differ Equ, 2006, 231: 252–289
[5] Rein G. Non-linear stability of gaseous stars. Arch Ration Mech Anal, 2003, 168(2): 115–130
[6] Luo T, Smoller J. Rotating fluids with self-gravitation in bounded domains. Arch Ration Mech Anal, 2004, 173 (3): 345–377
[7] Luo T, Smoller J. Existence and non-linear stability of rotating star solutions of the compressible Euler-Poisson equations. Arch Ration Mech Anal, 2009, 191: 447–496
[8] Liu T P, Yang T. Compressible flow with vacuum and physical singularity. Methods Appl Anal, 2000, 7: 495–510
[9] Gilbarg D, Trudinger N S. Elliptic Partial Differential Equations of Second Order. 2nd ed. Berlin, Heidel-berg, New York, Tokyo: Springer-Verlag, 1983
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