Slowly rotating relativistic stars. V. Static stability analysis of n=3/ 2 polytropes
Journal Article
·
· Astrophys. J., v. 198, no. 2, pp. 467-476
- Research Organization:
- Department of Physics, University of California, Santa Barbara
- Sponsoring Organization:
- USDOE
- NSA Number:
- NSA-32-026479
- OSTI ID:
- 4206012
- Journal Information:
- Astrophys. J., v. 198, no. 2, pp. 467-476, Other Information: Orig. Receipt Date: 31-DEC-75
- Country of Publication:
- United States
- Language:
- English
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Related Subjects
N56300* -Physics (Astrophysics & Cosmology)-Quasi-stellar
Radio & X-Ray Sources
640103* -Physics Research-Astrophysics & Cosmology-Quasi- Stellar
Radio & X-Ray Sources
*PULSARS- STABILITY
DENSITY
EQUILIBRIUM
FREQUENCY DEPENDENCE
NEUTRON STARS
OSCILLATIONS
PULSATIONS
RELATIVITY THEORY
ROTATION
Radio & X-Ray Sources
640103* -Physics Research-Astrophysics & Cosmology-Quasi- Stellar
Radio & X-Ray Sources
*PULSARS- STABILITY
DENSITY
EQUILIBRIUM
FREQUENCY DEPENDENCE
NEUTRON STARS
OSCILLATIONS
PULSATIONS
RELATIVITY THEORY
ROTATION