Radial oscillation spectra of an anisotropic strange quark star model of Cen X-3 are computed for three anisotropy prescriptions and differ by up to 40 percent between models.
Radial oscillations of zero-temperature white dwarfs and neutron stars below nuclear densities,
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On Modeling Anisotropic Quark Stars: The Role of Anisotropy in Radial Oscillation Spectra
Radial oscillation spectra of an anisotropic strange quark star model of Cen X-3 are computed for three anisotropy prescriptions and differ by up to 40 percent between models.