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astro-ph2004
Impact of the nuclear equation of state on the last orbits of binary neutron stars
M. Bejger, D. Gondek-Rosinska, E. Gourgoulhon +3
We present calculations of quasiequilibrium sequences of irrotational binary neutron stars based on realistic equations of state (EOS) for the whole neutron star interior. Three re…
astro-ph2004★ 14 cited
Surface gravity of neutron stars and strange stars
M. Bejger, P. Haensel
The upper bound on the value of the surface gravity, g_s, for neutron stars with equations of state respecting v_sound <= c, is derived. This bound is inversely proportional to the…