Newtonian hydrodynamics of the coalescence of black holes with neutron stars — III. Irrotational binaries with a stiff equation of state
Open Access
- 21 October 2000
- journal article
- research article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 318 (2) , 606-624
- https://doi.org/10.1046/j.1365-8711.2000.03870.x
Abstract
No abstract availableKeywords
All Related Versions
This publication has 82 references indexed in Scilit:
- Evolution of Binary Compact Objects That MergeThe Astrophysical Journal, 1998
- Binary Neutron Stars in General Relativity: Quasiequilibrium ModelsPhysical Review Letters, 1997
- von Neumann stability analysis of smoothed particle hydrodynamics—suggestions for optimal algorithmsJournal of Computational Physics, 1995
- Gravitational-Radiation Damping of Compact Binary Systems to Second Post-Newtonian OrderPhysical Review Letters, 1995
- Tidal interactions of inspiraling compact binariesThe Astrophysical Journal, 1992
- LIGO: The Laser Interferometer Gravitational-Wave ObservatoryScience, 1992
- Post-Newtonian hydrodynamics and post-Newtonian gravitational wave generation for numerical relativityMonthly Notices of the Royal Astronomical Society, 1990
- Dynamic mass exchange in doubly degenerate binaries. I - 0.9 and 1.2 solar mass starsThe Astrophysical Journal, 1990
- Electromagnetic extraction of energy from Kerr black holesMonthly Notices of the Royal Astronomical Society, 1977
- A Microscopic Interpretation of Neutron Star StructureThe Astrophysical Journal Supplement Series, 1977