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引用本文的文献

1
Rotating stars in relativity.
Living Rev Relativ. 2017;20(1):7. doi: 10.1007/s41114-017-0008-x. Epub 2017 Nov 29.

本文引用的文献

1
Quasi-Normal Modes of Stars and Black Holes.
Living Rev Relativ. 1999;2(1):2. doi: 10.12942/lrr-1999-2. Epub 1999 Sep 16.
2
Gravitational Waves and Pulsating Stars: What Can We Learn from Future Observations?
Phys Rev Lett. 1996 Nov 11;77(20):4134-4137. doi: 10.1103/PhysRevLett.77.4134.
3
Kaon energies in dense matter.
Phys Rev Lett. 1995 Dec 18;75(25):4567-4570. doi: 10.1103/PhysRevLett.75.4567.
4
Gravitational radiation from nonaxisymmetric instability in a rotating star.
Phys Rev Lett. 1994 Feb 28;72(9):1314-1317. doi: 10.1103/PhysRevLett.72.1314.
5
Direct URCA process in neutron stars.
Phys Rev Lett. 1991 May 27;66(21):2701-2704. doi: 10.1103/PhysRevLett.66.2701.
6
Implications of a half-millisecond pulsar.
Phys Rev Lett. 1989 Jun 26;62(26):3015-3019. doi: 10.1103/PhysRevLett.62.3015.
8
Equations governing the nonradial oscillations of a slowly rotating relativistic star.
Phys Rev D Part Fields. 1992 Nov 15;46(10):4289-4303. doi: 10.1103/physrevd.46.4289.
9
Limiting rotational period of neutron stars.
Phys Rev D Part Fields. 1992 Nov 15;46(10):4161-4168. doi: 10.1103/physrevd.46.4161.
10
Relation of gauge formalisms for pulsations of general-relativistic stellar models.
Phys Rev D Part Fields. 1991 Jul 15;44(2):307-313. doi: 10.1103/physrevd.44.307.

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