[1] Abdallah M A, Jiang F, Tan Z. Decay estimates for isentropic compressible magnetohydrodynamic equations in bounded domain. Acta Math Sci, 2012, 32B(6):2211-2220
[2] Chen G Q, Wang D H. Global solution of nonlinear magnetohydrodynamics with large initial data. J Differential Equations, 2002, 182:344-376
[3] Cox J P, Giuli R T. Principles of Stellar Structure, I, II. New York:Gordon and Breach, 1968
[4] Chen G Q, Wang D H. Existence and continuous dependence of large solutions for the magnetohydrodynamic equations. Z Angew Math Phys, 2003, (54):608-632
[5] Duan Q, Li H L. Global existence of weak solution for the compressible Navier-Stokes-Poisson system for gaseous stars. J Differential Equations, 2015, 259(10):5302-5330
[6] Duan R J, Ruan L Z, Zhu C J. Optimal decay rates to conservation laws with diffusion-type terms of regularity-gain and regularity-loss. Math Models Methods Appl Sci, 2012, 22(07):1250012
[7] Duan R J, Ukai S, Yang T, Zhao H J. Optimal convergence rates for the compressible Navier-Stokes equations with potential forces. Math Models Methods Appl Sci, 2007, 17(5):737-758
[8] Fan J S, Jiang S, Nakamura G. Vanishing shear viscosity limit in the magnetohydrodynamic equations. Comm Math Phys, 2007, 270:691-708
[9] Fan J S, Yu W H. Global variational solutions to the compressible magnetohydrodynamic equations. Nonlinear Anal, 2008, 69:3637-3660
[10] Fan J S, Yu W H. Strong solution to the compressible magnetohydrodynamic equations with vacuum. Nonlinear Anal Real World Appl, 2009, (10):392-409
[11] Federbush P, Luo T, Smoller J. Existence of magnetic compressible fluid stars. Arch Rational Mech Anal, 2015, 215(2):611-631
[12] Feireisl E, Novotný A, Petleltová H. On the existence of globally defined weak solutions to the Navier-Stokes equations of isentropic compressible fluids. J Math Fluid Mech, 2001, (3):358-392
[13] Hao C, Li H L. Global existence for compressible Navier-Stokes-Poisson equations in three and higher dimensions. J Differential Equations, 2009, 246(12):4791-4812
[14] Hong G, Luo T, Zhu C. Global solutions to physical vacuum problem of non-isentropic viscous gaseous stars and nonlinear asymptotic stability of stationary solutions. J Differential Equations, 2018, 265(1):177-236
[15] Hu X P, Wang D H. Global solutions to the three-dimensional full compressible magnetohydrodynamic flows. Comm Math Phys, 2008, 283:255-284
[16] Hu X P, Wang D H. Global existence and large-time behavior of solutions to the three-dimensional equations of compressible magnetohydrodynamic flows. Arch Ration Mech Anal, 2010, 197:203-238
[17] Jang J, Strauss W A, Wu Y. Existence of rotating magnetic stars. Physica D:Nonlinear Phenomena, 2019, 397:65-74
[18] Jiang M, Lai S, Yin H, Zhu C. The stability of stationary solution for outflow problem on the NavierStokes-Poisson system. Acta Math Sci, 2016, 36B(4):1098-1116
[19] Kong H, Li H L. Free boundary value problem to 3D spherically symmetric compressible Navier-StokesPoisson equations. Zeitschrift für Angewandte Mathematik und Physik, 2017, 68(1):21
[20] Li H L, Matsumura A, Zhang G. Optimal Decay Rate of the Compressible Navier-Stokes-Poisson System in $\mathbb{R}^3$. Arch Rational Mech Anal, 2010, 196(2):681-713
[21] Li H L, Xu X Y, Zhang J W. Global classical solutions to 3D compressible magnetohydrodynamic equations with large oscillations and vacuum. SIAM J Math Anal, 2013, 45:1356-1387
[22] Li F C, Yu H J. Optimal decay rate of classical solutions to the compressible magnetohydrodynamic equations. Proc Roy Soc Edinburgh Sect A, 2011, 141:109-126
[23] Li H L, Zhang T. Large time behavior of solutions to 3D compressible Navier-Stokes-Poisson system. Science China Mathematics, 2012, 55(1):159-177
[24] Lions P L. Mathematical Topics in Fluids Mechanics. New York:Oxford University Press, 1998
[25] Luo T, Xin Z P, Zeng H. Nonlinear asymptotic stability of the Lane-Emden solutions for the viscous gaseous star problem with degenerate density dependent viscosities. Comm Math Phys, 2016, 347:657-702
[26] Luo T, Xin Z P, Zeng H. On nonlinear asymptotic stability of the Lane-Emden solutions for the viscous gaseous star problem. Adv Math, 2016, 291:90-182
[27] Shapiro S H, Teukolsky S A. Black Holes, White Dwarfs, and Neutron Stars. New York:Wiley-Vch, 2004
[28] Tan Z, Tong L L, Wang Y. Large time behavior of the compressible magnetohydrodynamic equations with Coulomb force. J Math Anal Appl, 2015, 427:600-617
[29] Tan Z, Wang Y J. Global existence and large-time behavior of weak solutions to the compressible magnetohydrodynamic equations with Coulomb force. Nonlinear Anal, 2009, 71:5866-5884
[30] Wang D H. Large solutions to the initial-boundary value problem for planar magnetohydrodynamics. SIAM J Appl Math, 2003, 63:1424-1441
[31] Wang H, Liu R. The existence of stationary star solutions for compressible magnetohydrodynamic flows. Boundary Value Problems, 2016, 2016(1):216
[32] Wang W K, Wu Z G, Pointwise estimates of solution for the Navier-Stokes-Poisson equations in multidimensions. J Differential Equations, 2010, 248:1617-1636
[33] Wang Y Z, Wang K Y. Asymptotic behavior of classical solutions to the compressible Navier-Stokes-Poisson equations in three and higher dimensions. J Differential Equations, 2015, 259:25-47
[34] Yang J. Quasi-neutral limit of Euler-Poisson system of compressible fluids coupled to a magnetic field. Zeitschrift Für Angewandte Mathematik Und Physik, 2018, 69(3):73
[35] Zirin H. Astrophysics of the Sun. Cambridge:Cambridge University Press, 1988
