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Simulations of Binary Coalescence of a Neutron Star and a Black Hole

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Published 1998 January 9 © 1998. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation W. Kluźniak and W. H. Lee 1998 ApJ 494 L53 DOI 10.1086/311151

1538-4357/494/1/L53

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.

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10.1086/311151