On the limiting mass of neutron stars
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The maximum mass of neutron stars is one of the most important predictions of the general relativistic theory of stellar structure. This paper highlights the difficulties in making a definitive prediction, and also reviews the progress made so far.
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Black Holes in Binaries and Galactic Nuclei: Diagnostics, Demography and Formation: Proceedings of the ESO Workshop Held at Garching, Germany, 6-8 September 1999, in Honour of Riccardo Giacconi, ESO ASTROPHYSICS SYMPOSIA. Eds. L. Kaper, E.P.J. van den Heuvel, and P.A. Woudt. p45, Springer-Verlag, 2001.
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2001 Springer-Verlag