Slowly Rotating Relativistic Stars. I. Equations of Structure
Abstract
Equations are given for the calculation of the equilibrium configurations of slowly rotating stars in the framework of general relativity. The rotation is treated to second order in the angular velocity, but no other approximation is made.
- Publication:
-
The Astrophysical Journal
- Pub Date:
- December 1967
- DOI:
- 10.1086/149400
- Bibcode:
- 1967ApJ...150.1005H