Low density neutron star model for CEN X-3 and HER X-1

Astronomy and Astrophysics – Astronomy

Scientific paper

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Astronomical Models, Binary Stars, Neutron Stars, Nuclear Binding Energy, Stellar Rotation, X Ray Sources, Density (Mass/Volume), Dynamic Stability, Equations Of State, Stellar Mass, X Ray Stars

Scientific paper

It is suggested that rotating low-density neutron stars undergoing
accretion can account for many of the features of Cen X-3 and Her X-1.
The binding energies of such stars are computed for several equations of
state. All the computed models are bound with respect to O-16,
indicating that they might be formed in close binary systems.

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