Results 141 to 143 of about 4,836 (143)

Magnetohydrodynamic Oscillations of Neutron Stars

Nature Physical Science, 1971
FLUID motions in neutron stars have been investigated theoretically several times1–3, but the problem of free magnetohydrodynamic oscillations has evidently not been considered previously, notwithstanding its possible importance in connexion with the interpretation of pulsar observations4–7, especially the modulation of pulse rates8,9.
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Rotating and Oscillating Neutron Stars

1996
Since neutron stars are extremely compact objects with strong gravity, general relativity must be employed in modelling their properties. The structure and gravitational fields of spherically symmetric, nonrotating stars are governed by the Tolman-Oppenheimer-Volkoff equations, a set of ordinary differential equations.
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Oscillations of a star with a phase transition

Astrophysics, 1984
Z. F. Seidov, G. S. Bisnovatyi-Kogan
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