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arXiv · astro-ph/9711172

Black hole neutron star coalescence as a source of gamma-ray bursts

W. H. Lee·W. Kluzniak
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Abstract

We present the results of hydrodynamic (SPH) simulations showing the coalescence of a black hole with a neutron star to be a promising theoretical source of short duration gamma-ray bursts. The favorable features of the process include rapid onset, millisecond variability, a duration much longer than the dynamical timescale, and a range of outcomes sufficient to allow variety in the properties of individual gamma-ray bursts. Interestingly, the process of coalescence differs rather markedly from past predictions.

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W. H. Lee, W. Kluzniak. 1997-11-14. Black hole neutron star coalescence as a source of gamma-ray bursts. https://doi.org/10.1063/1.55453

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