Instability of Synchronized Binary Neutron Stars in the First Post-Newtonian Approximation of General Relativity
- 1 August 1996
- journal article
- Published by Oxford University Press (OUP) in Progress of Theoretical Physics
- Vol. 96 (2) , 317-325
- https://doi.org/10.1143/ptp.96.317
Abstract
No abstract availableKeywords
This publication has 1 reference indexed in Scilit:
- Ellipsoidal figures of equilibrium - Compressible modelsThe Astrophysical Journal Supplement Series, 1993