Neutron star models |
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| Authors: | Gerhard Börner Katsuhiko Sato |
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| Institution: | (1) Physics Dept., City College, New York, USA;(2) Physics Dept., Kyoto University, Kyoto, Japan;(3) Present address: Max-Planck-Institut für Physik und Astrophysik, München |
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| Abstract: | Neutron star models are calculated using an equation of state discussed in an earlier paper. A maximum mass for a neutron star of 1.74 solar masses is found. The central density of thie star is 3.3×1015 g/cm3. The lightest stars have masses of 0.02 (resp. 0.03) solar masses with central densities 2.2×1014 g/cm3 (resp. 1.9×1014). |
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