HER X-1 and CEN X-3 revisited

Details HER X-1 and CEN X-3 revisited HER X-1 and CEN X-3 revisited

Oct 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975nyasa.262..312g&link_type=abstract

(AAS, American Physical Society, and New York Academy of Sciences, Texas Symposium on Relativistic Astrophysics, 7th, Dallas, Te

Astronomy and Astrophysics

Astronomy

19

Astronomical Models, Neutron Stars, Pulsed Radiation, Stellar Winds, X Ray Stars, Emission Spectra, Gravitational Collapse, Light Curve, Stellar Gravitation, X Ray Astronomy, X Ray Sources

Scientific paper

A model is developed which assumes that Cen X-3 and Her X-1 are magnetized neutron stars that accrete matter from a normal companion. Cen X-3 is an extar that receives mass from the companion through radiation-driven stellar winds, while Her X-1 receives mass through Roche lobe overflow. X-ray observations of these two systems have been analyzed to test this model. Large-scale effects related to eclipse and accretion are considered, as well as small-scale effects related to pulsation.

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