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The First Steps in the Life of a GRB

Published online by Cambridge University Press:  19 September 2016

Miguel A. Aloy*
Affiliation:
Max-Planck-Institut für Astrophysik, Karl-Schwarzschild-Str. 1, 85741 Garching, Germanymaa@mpa-garching.mpg.de

Summary

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We present some preliminary results of relativistic hydrodynamic simulations of post-neutron star merger disks as potential candidates for progenitors of short-lasting gamma-ray bursts. We discuss some of the generic conditions under which a gamma-ray burst can be initiated in this kind of progenitor and the main characteristics of the resulting outflow.

Type
Part VII Gamma-Ray Bursters
Copyright
Copyright © Springer-Verlag 2005

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