Turning-point method for axisymmetric stability of rotating relativistic stars

• 1 February 1988
• journal article
• Published by American Astronomical Society in The Astrophysical Journal
• Vol. 325, 722-724
• https://doi.org/10.1086/166043

Abstract

Keywords

• RELATIVISTIC VELOCITY
• STELLAR MOTIONS
• STELLAR ROTATION
• ANGULAR MOMENTUM
• NEUTRON STARS
• PERTURBATION THEORY
• POLYTROPIC PROCESSES
• SECULAR VARIATIONS