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Dynamical Stability of Neutron Stars

Published online by Cambridge University Press:  07 February 2017

G. Chanmugam  and
M. Gabriel
G. Chanmugam
Affiliation:
Institut d'Astrophysique, Université de Liège, B4200 Cointe-Ougree, Belgium
M. Gabriel
Affiliation:
Institut d'Astrophysique, Université de Liège, B4200 Cointe-Ougree, Belgium

Abstract

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The Nemeth-Sprung equation of state is modified and used to obtain neutron star models. Contrary to the results of some authors it is found that neutron stars with central densities ≲ 1014 g cm-3 are dynamically stable. It is suggested that some pulsars may belong to this category of stars.

Type
Session 6
Information
Symposium - International Astronomical Union , Volume 46: The Crab Nebula , 1971 , pp. 341 - 345
Copyright
Copyright © Reidel 1971 

References

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