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

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

Aug 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976mnras.176..315c&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 176, Aug. 1976, p. 315-320.

Astronomy and Astrophysics

Astronomy

1

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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