Fast Rotation of Neutron Stars

Astronomy and Astrophysics – Astrophysics

Scientific paper

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12 pages, LateX, uses aaspp.sty file, figures (Postscript files) available from haensel@camk.edu.pl; to be published in the As

Scientific paper

10.1086/176650

We show that for realistic equations of state of dense matter, the universal proportionality factor relating the maximum rotation rate of neutron stars due to mass-shedding limit to the mass and radius of maximum allowable mass configuration of non-rotating models results from a universal proportionality between masses and radii of static maximum-mass neutron stars and those of maximally rotating configurations. These empirical relations cannot be obtained in the slow rotation approximation.

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