Mass-radius relations of X-ray pulsars.

Details Mass-radius relations of X-ray pulsars. Mass-radius relations of X-ray pulsars.

Feb 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996rftu.proc..159l&link_type=abstract

International Conference on X-ray Astronomy and Astrophysics: Röntgenstrahlung from the Universe, p. 159 - 160

Astronomy and Astrophysics

Astrophysics

X-Ray Pulsars: Mass-Radius Relation

Scientific paper

The semi-empirical mass-radius (M-R) relations of four X-ray pulsars, Cen X-3, 4U 1626-67, Her X-1 and EXO 2030+375, are calculated, based on the observed data and the authors' accretion torque model. Comparison between the semi-empirical and the theoretical M-R relations shows that Cen X-3, 4U 1626-67 and EXO 2030+375, are consistent with the stiff or intermediate stiff equations of state, while Her X-1 seems not to be well described by the standard equations of state, though it may reconcile with the soft equation of state.

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