Axisymmetric modes of rotating relativistic stars in the Cowling approximation
Open Access
- 21 August 2001
- journal article
- research article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 325 (4) , 1463-1470
- https://doi.org/10.1046/j.1365-8711.2001.04555.x
Abstract
No abstract availableKeywords
All Related Versions
This publication has 24 references indexed in Scilit:
- The Piecewise Parabolic Method (PPM) for gas-dynamical simulationsPublished by Elsevier ,2004
- Towards a stable numerical evolution of strongly gravitating systems in general relativity: The conformal treatmentsPhysical Review D, 2000
- Numerical Hydrodynamics in General RelativityLiving Reviews in Relativity, 2000
- A Flux-Split Algorithm Applied to Relativistic FlowsJournal of Computational Physics, 1998
- RADIAL MODES OF ROTATING NEUTRON STARS IN THE CHANDRASEKHAR–FRIEDMAN FORMALISMInternational Journal of Modern Physics D, 1998
- Gravitational Waves from Phase Transitions of Accreting Neutron StarsThe Astrophysical Journal, 1998
- Numerical {3 + 1} General Relativistic Hydrodynamics: A Local Characteristic ApproachThe Astrophysical Journal, 1997
- Normal modes of oscillation for rotating stars. III - Variational calculations with an improved set of basis vectorsThe Astrophysical Journal, 1986
- Normal modes of oscillation for rotating stars. II Variational solutionsThe Astrophysical Journal, 1984
- Normal modes of oscillation for rotating stars. I - The effect of rigid rotation on four low-order pulsationsThe Astrophysical Journal, 1981