Slowly Rotating Relativistic Stars.VI. Stability of the Quasiradial Modes
Abstract
Equations are given for calculating the effects of a slow and rigid rotation on the frequency of the radial modes of oscillation of a relativistic star. The rotation is treated to second order in the angular velocity, but no other approximations are made.
- Publication:
-
The Astrophysical Journal
- Pub Date:
- August 1972
- DOI:
- 10.1086/151620
- Bibcode:
- 1972ApJ...176..177H