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• W3103210010 abstract "We present the results of Newtonian hydrodynamic simulations of the coalescence of a binary consisting of a black hole with a neutron star. The calculations show that for a wide range of initial conditions the core of the neutron star survives the initial mass transfer episode. We therefore identify black hole-neutron star binaries as the astrophysical production site of low-mass neutron stars unstable to explosion. The relevance of the simulations to the theory of gamma-ray bursts is also discussed." @default.
• W3103210010 created "2020-11-23" @default.
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• W3103210010 date "1998-02-10" @default.
• W3103210010 modified "2023-10-18" @default.
• W3103210010 title "Simulations of Binary Coalescence of a Neutron Star and a Black Hole" @default.
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• W3103210010 doi "https://doi.org/10.1086/311151" @default.
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